[{"height": 1650, "img_url": "snowmtl.ru/latest/the-original/205/0.webp", "translations": [{"angle": 0, "bbox": ["18", "1134", "226", "1299"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "DE TOUTE FA\u00c7ON, ILS NE PEUVENT PAS ME BLESSER, ALORS QU\u0027EST-CE QUE \u00c7A PEUT FAIRE S\u0027ILS ME PIQUENT UN PEU...", "id": "Toh mereka tidak bisa melukaiku, biarkan saja mereka menusuk beberapa kali, apa salahnya...", "is_bold": false, "pt": "DE QUALQUER FORMA, ELES N\u00c3O PODEM ME MACHUCAR. QUAL O PROBLEMA DE DEIX\u00c1-LOS ME ATACAR ALGUMAS VEZES...", "text": "ANYWAY, THEY CAN\u0027T HURT ME, SO WHAT DOES IT MATTER IF THEY POKE ME A FEW TIMES...", "tr": "Nas\u0131lsa bana zarar veremezler, birka\u00e7 kez d\u00fcrtmelerinin ne sak\u0131ncas\u0131 var ki...", "type": "inside"}, {"angle": 0, "bbox": ["897", "1172", "1059", "1332"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "BIEN QU\u0027ILS SOIENT EN EFFET UN PEU PLUS FORTS QU\u0027AVANT.", "id": "Meskipun mereka memang sedikit lebih kuat dari sebelumnya.", "is_bold": false, "pt": "EMBORA SEJAM DE FATO UM POUCO MAIS FORTES DO QUE ANTES.", "text": "ALTHOUGH THEY ARE INDEED A BIT STRONGER THAN BEFORE.", "tr": "Ger\u00e7i \u00f6ncekilerden biraz daha g\u00fc\u00e7l\u00fcler.", "type": "inside"}, {"angle": 0, "bbox": ["800", "1357", "974", "1489"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "ILS PEUVENT PERCER MON ARMURE ORIGINELLE.", "id": "Bisa menembus armor asliku.", "is_bold": false, "pt": "CONSEGUEM PERFURAR MINHA ARMADURA PRIMORDIAL.", "text": "THEY CAN PIERCE MY PRIMAL ARMOR.", "tr": "Orijinal z\u0131rh\u0131m\u0131 delebiliyorlar.", "type": "inside"}, {"angle": 1.6632633872859515e-05, "bbox": ["867", "446", "994", "483"], "bg_color": ["44", "44", "44"], "fg_color": ["124", "124", "124"], "fr": "VENEZ !", "id": "Ayo!", "is_bold": false, "pt": "VENHAM!", "text": "COME ON!", "tr": "Gelin bakal\u0131m!", "type": "outside"}, {"angle": 2.0751079460978872e-05, "bbox": ["861", "494", "1037", "532"], "bg_color": ["41", "41", "41"], "fg_color": ["118", "118", "118"], "fr": "VERMINES !", "id": "Sampah!", "is_bold": false, "pt": "SEUS VERMES!", "text": "WEAKLINGS!", "tr": "Ez\u00fckler!", "type": "outside"}, {"angle": 0.0012364175608503016, "bbox": ["734", "595", "1028", "629"], "bg_color": ["27", "27", "27"], "fg_color": ["116", "116", "116"], "fr": "\u00c7A NE FAIT PAS MAL DU TOUT ! VERMINES !", "id": "Tidak sakit sama sekali! Sampah!", "is_bold": false, "pt": "N\u00c3O D\u00d3I NADA! SEUS VERMES!", "text": "DOESN\u0027T HURT AT ALL! WEAKLINGS!", "tr": "Hi\u00e7 ac\u0131m\u0131yor! Ez\u00fckler!", "type": "outside"}, {"angle": 3.5511869214133185e-06, "bbox": ["741", "631", "937", "658"], "bg_color": ["32", "32", "32"], "fg_color": ["117", "117", "117"], "fr": "VENEZ TOUS ! VENEZ !", "id": "Ayo semua! Ayo!", "is_bold": false, "pt": "VENHAM TODOS! VENHAM!", "text": "COME ON! ALL OF YOU!", "tr": "Hepiniz gelin! Gelin!", "type": "outside"}], "width": 1080}, {"height": 1050, "img_url": "snowmtl.ru/latest/the-original/205/1.webp", "translations": [{"angle": 0, "bbox": ["252", "66", "498", "199"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "CES B\u00caTES ORIGINELLES NE PEUVENT BIEN S\u00dbR PAS VOUS BLESSER.", "id": "Monster-monster ini tentu saja tidak bisa melukai kalian.", "is_bold": false, "pt": "ESSAS BESTAS PRIMORDIAIS CERTAMENTE N\u00c3O PODEM FERIR VOC\u00caS.", "text": "OF COURSE, THESE PRIMAL BEASTS CAN\u0027T HURT YOU.", "tr": "Bu \u0130lkel Canavarlar tabii ki size zarar veremez.", "type": "inside"}, {"angle": 0, "bbox": ["23", "698", "210", "839"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "VOUS COMBATTIEZ \u00c0 L\u0027INSTANT DANS UNE ZONE CONTR\u00d4L\u00c9E.", "id": "Kalian tadi bertarung dalam jangkauan yang terkendali.", "is_bold": false, "pt": "VOC\u00caS ESTAVAM LUTANDO DENTRO DE UMA \u00c1REA CONTROLADA AGORA H\u00c1 POUCO.", "text": "YOU WERE JUST FIGHTING WITHIN CONTROLLED PARAMETERS.", "tr": "Az \u00f6nce kontroll\u00fc bir alanda sava\u015f\u0131yordunuz.", "type": "inside"}, {"angle": 0, "bbox": ["622", "766", "819", "917"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "LEUR VALEUR DE D\u00c9G\u00c2TS MAXIMALE A \u00c9T\u00c9 AJUST\u00c9E POUR NE PAS VOUS BLESSER.", "id": "Nilai kerusakan maksimum mereka sudah dipastikan tidak bisa melukai kalian.", "is_bold": false, "pt": "O DANO M\u00c1XIMO DELAS FOI AJUSTADO PARA GARANTIR QUE N\u00c3O OS FERISSEM.", "text": "THEIR MAXIMUM DAMAGE OUTPUT WAS ENSURED NOT TO HARM YOU.", "tr": "Maksimum hasar de\u011ferleri size zarar vermeyecek \u015fekilde ayarlanm\u0131\u015ft\u0131.", "type": "inside"}], "width": 1080}, {"height": 600, "img_url": "snowmtl.ru/latest/the-original/205/2.webp", "translations": [{"angle": 0, "bbox": ["24", "26", "215", "182"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "MAIS EN COMBAT R\u00c9EL, RIEN DE TOUT CELA N\u0027EST GARANTI.", "id": "Tapi dalam pertarungan sungguhan, semua ini tidak bisa dijamin.", "is_bold": false, "pt": "MAS EM COMBATE REAL, NADA DISSO PODE SER GARANTIDO.", "text": "BUT IN A REAL BATTLE, NONE OF THIS CAN BE GUARANTEED.", "tr": "Ama ger\u00e7ek bir sava\u015fta bunlar\u0131n hi\u00e7biri garanti edilemez.", "type": "inside"}, {"angle": 0, "bbox": ["545", "58", "639", "127"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "COMPRIS ?", "id": "Paham?", "is_bold": false, "pt": "ENTENDERAM?", "text": "UNDERSTAND?", "tr": "Anlad\u0131n\u0131z m\u0131?", "type": "inside"}, {"angle": 0, "bbox": ["729", "26", "985", "154"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "MAIS... MAIS NOUS AVONS D\u00c9J\u00c0 TU\u00c9 UN NID DE B\u00caTES ORIGINELLES AVANT !", "id": "Tapi, tapi kita sebelumnya juga sudah membunuh satu sarang monster!", "is_bold": false, "pt": "MAS... MAS N\u00d3S J\u00c1 MATAMOS UM NINHO DE BESTAS PRIMORDIAIS ANTES!", "text": "BUT... BUT WE KILLED A NEST OF PRIMAL BEASTS BEFORE!", "tr": "Ama... ama daha \u00f6nce bir s\u00fcr\u00fc \u0130lkel Canavar \u00f6ld\u00fcrm\u00fc\u015ft\u00fck!", "type": "inside"}, {"angle": 0, "bbox": ["872", "158", "1056", "308"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "EST-CE QUE C\u0027\u00c9TAIT AUSSI CALCUL\u00c9 PAR VOUS ?", "id": "Apa itu juga sudah kalian perhitungkan?", "is_bold": false, "pt": "AQUILO TAMB\u00c9M FOI CALCULADO POR VOC\u00caS?", "text": "WAS THAT ALSO PART OF YOUR CALCULATIONS?", "tr": "Yoksa o da m\u0131 sizin hesab\u0131n\u0131zdayd\u0131?", "type": "inside"}], "width": 1080}, {"height": 1650, "img_url": "snowmtl.ru/latest/the-original/205/3.webp", "translations": [{"angle": 0, "bbox": ["86", "324", "255", "477"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "REGARDONS D\u0027ABORD UNE VID\u00c9O.", "id": "Mari kita lihat rekaman video dulu.", "is_bold": false, "pt": "PRIMEIRO, VAMOS ASSISTIR A UMA GRAVA\u00c7\u00c3O.", "text": "LET\u0027S WATCH A RECORDING FIRST.", "tr": "\u00d6nce bir video izleyelim.", "type": "inside"}, {"angle": 0, "bbox": ["795", "1121", "971", "1272"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "INSTRUCTEUR ! ! !", "id": "Instruktur!!!", "is_bold": false, "pt": "INSTRUTOR!!!", "text": "INSTRUCTOR!!!", "tr": "E\u011fitmen!!!", "type": "inside"}, {"angle": 0, "bbox": ["923", "568", "1056", "655"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "C\u0027EST !", "id": "Ini!", "is_bold": false, "pt": "ISTO \u00c9!", "text": "THIS IS!", "tr": "Bu!", "type": "inside"}], "width": 1080}, {"height": 1125, "img_url": "snowmtl.ru/latest/the-original/205/4.webp", "translations": [{"angle": 0, "bbox": ["21", "77", "228", "220"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "C\u0027EST UNE MISSION D\u0027IL Y A PLUS DE QUARANTE ANS.", "id": "Ini adalah misi lebih dari empat puluh tahun yang lalu.", "is_bold": false, "pt": "ESTA FOI UMA MISS\u00c3O DE MAIS DE QUARENTA ANOS ATR\u00c1S.", "text": "THIS IS A MISSION FROM OVER FORTY YEARS AGO.", "tr": "Bu, k\u0131rk k\u00fcsur y\u0131l \u00f6nceki bir g\u00f6rev.", "type": "inside"}, {"angle": 0, "bbox": ["76", "274", "237", "405"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "\u00c0 L\u0027\u00c9POQUE, J\u0027\u00c9TAIS NIVEAU QUATRE.", "id": "Saat itu aku level empat.", "is_bold": false, "pt": "NAQUELA \u00c9POCA, EU ERA N\u00cdVEL QUATRO.", "text": "I WAS LEVEL 4 BACK THEN.", "tr": "O zamanlar d\u00f6rd\u00fcnc\u00fc seviyedeydim.", "type": "inside"}, {"angle": 0, "bbox": ["21", "938", "233", "1101"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "LA CIBLE \u00c9TAIT AUSSI UNE B\u00caTE ORIGINELLE DE NIVEAU DEUX.", "id": "Target saat itu juga monster level dua.", "is_bold": false, "pt": "O ALVO NA \u00c9POCA TAMB\u00c9M ERA UM PRIMORDIAL DE N\u00cdVEL DOIS.", "text": "THE TARGET THEN WAS ALSO A LEVEL 2 PRIMAL EYE.", "tr": "O zamanki hedef de ikinci seviye bir \u0130lkel Odak\u0027t\u0131.", "type": "inside"}, {"angle": 0, "bbox": ["892", "632", "1058", "755"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "MAIS CES B\u00caTES ORIGINELLES N\u0027\u00c9TAIENT PAS TOUTES DE NIVEAU DEUX.", "id": "Tapi monster-monster itu tidak semuanya level dua.", "is_bold": false, "pt": "MAS AQUELAS BESTAS PRIMORDIAIS N\u00c3O ERAM TODAS DE N\u00cdVEL DOIS.", "text": "BUT THOSE PRIMAL BEASTS WEREN\u0027T ALL LEVEL 2.", "tr": "Ama o \u0130lkel Canavarlar\u0131n hepsi ikinci seviye de\u011fildi.", "type": "inside"}, {"angle": -0.03980148102465364, "bbox": ["600", "646", "737", "723"], "bg_color": ["147", "146", "139"], "fg_color": ["119", "120", "112"], "fr": "[SFX] PAF !", "id": "[SFX] PLAK!", "is_bold": false, "pt": "[SFX] PLAFT!", "text": "SMACK!", "tr": "[SFX] PAT!", "type": "sfx"}], "width": 1080}, {"height": 525, "img_url": "snowmtl.ru/latest/the-original/205/5.webp", "translations": [{"angle": -0.33682955193575026, "bbox": ["752", "241", "939", "408"], "bg_color": ["167", "155", "119"], "fg_color": ["145", "140", "119"], "fr": "ANALYSE", "id": "Terlepas.", "is_bold": false, "pt": "[SFX] CLIQUE!", "text": "", "tr": "[SFX] \u00c7\u00f6z\u00fclme!", "type": "outside"}], "width": 1080}, {"height": 1650, "img_url": "snowmtl.ru/latest/the-original/205/6.webp", "translations": [{"angle": 0, "bbox": ["456", "73", "738", "223"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "DES B\u00caTES ORIGINELLES DE HAUT NIVEAU VENUES D\u0027AILLEURS S\u0027Y M\u00caLENT SOUVENT...", "id": "Monster level tinggi dari tempat lain sering bercampur di antara mereka...", "is_bold": false, "pt": "BESTAS PRIMORDIAIS DE N\u00cdVEL SUPERIOR VINDAS DE OUTROS LUGARES COSTUMAM SE MISTURAR ENTRE ELAS...", "text": "HIGHER-LEVEL PRIMAL BEASTS FROM ELSEWHERE OFTEN MIXED IN...", "tr": "Ba\u015fka yerlerden gelen y\u00fcksek seviyeli \u0130lkel Canavarlar s\u0131k s\u0131k aralar\u0131na kar\u0131\u015f\u0131r...", "type": "inside"}], "width": 1080}, {"height": 75, "img_url": "snowmtl.ru/latest/the-original/205/7.webp", "translations": [], "width": 1080}, {"height": 1650, "img_url": "snowmtl.ru/latest/the-original/205/8.webp", "translations": [{"angle": 0, "bbox": ["844", "18", "1058", "178"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "D\u0027AILLEURS, QU\u0027EST-CE QUI T\u0027A TU\u00c9 EN UN COUP ?!", "id": "Ngomong-ngomong, apa yang membunuhmu dalam sekejap itu?!", "is_bold": false, "pt": "FALANDO NISSO, O QUE FOI AQUILO QUE TE MATOU INSTANTANEAMENTE?!", "text": "SPEAKING OF WHICH, WHAT WAS THAT THING THAT INSTA-KILLED YOU?!", "tr": "Bu arada, seni an\u0131nda \u00f6ld\u00fcren \u015fey neydi?!", "type": "inside"}, {"angle": 0, "bbox": ["22", "677", "208", "825"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "POURQUOI EST-CE SI FLOU ?", "id": "Kenapa buram sekali?", "is_bold": false, "pt": "POR QUE EST\u00c1 T\u00c3O EMBA\u00c7ADO?", "text": "WHY IS IT SO BLURRY?", "tr": "Neden bu kadar bulan\u0131k?", "type": "inside"}, {"angle": 0, "bbox": ["872", "677", "1057", "801"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "VOUS L\u0027AVEZ CENSUR\u00c9 ?", "id": "Apa kalian menyensornya?", "is_bold": false, "pt": "VOC\u00caS CENSURARAM?", "text": "DID YOU CENSOR IT?", "tr": "Sans\u00fcrlediniz mi?", "type": "inside"}, {"angle": 0, "bbox": ["78", "1044", "390", "1208"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "LES CAM\u00c9RAS HAUTE D\u00c9FINITION DE NIVEAU MAGN\u00c9TO-ORIGINEL SONT AFFECT\u00c9ES.", "id": "Kamera level medan magnetik tinggi akan terpengaruh.", "is_bold": false, "pt": "C\u00c2MERAS DE ALTA DEFINI\u00c7\u00c3O S\u00c3O AFETADAS PELO N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL.", "text": "HIGH PRIMAL MAGNETIC LEVELS AFFECT CAMERAS.", "tr": "Y\u00fcksek \u0130lkel Manyetik Seviyeler, kameralar\u0131 etkiler.", "type": "inside"}, {"angle": 0, "bbox": ["848", "1410", "1058", "1569"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "NIVEAU MAGN\u00c9TO-ORIGINEL ?!", "id": "Level medan magnetik?!", "is_bold": false, "pt": "N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL?!", "text": "PRIMAL MAGNETIC LEVEL?!", "tr": "\u0130lkel Manyetik Seviye?!", "type": "inside"}], "width": 1080}, {"height": 1075, "img_url": "snowmtl.ru/latest/the-original/205/9.webp", "translations": [{"angle": 0, "bbox": ["21", "26", "264", "205"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "LES PRIMAL EYES, LES B\u00caTES ORIGINELLES, Y COMPRIS NOUS, LES VARIANTS ORIGINELS...", "id": "Monster, monster buas, termasuk kita para mutan,", "is_bold": false, "pt": "PRIMORDIAIS, BESTAS PRIMORDIAIS, E INCLUINDO N\u00d3S, OS METAMORFOS PRIMORDIAIS...", "text": "PRIMAL EYES, PRIMAL BEASTS, INCLUDING US PRIMORDIAL VARIANTS...", "tr": "\u0130lkel Odaklar, \u0130lkel Canavarlar ve biz \u0130lkel Varyantlar dahil olmak \u00fczere,", "type": "inside"}, {"angle": 0, "bbox": ["162", "210", "348", "361"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "...ONT TOUS UN CHAMP MAGN\u00c9TIQUE SP\u00c9CIAL.", "id": "Semuanya memiliki medan magnet khusus.", "is_bold": false, "pt": "TODOS POSSUEM UM CAMPO MAGN\u00c9TICO ESPECIAL.", "text": "...ALL HAVE A SPECIAL MAGNETIC FIELD.", "tr": "hepsinin \u00f6zel bir manyetik alan\u0131 vard\u0131r.", "type": "inside"}, {"angle": 0, "bbox": ["784", "82", "988", "258"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "APPEL\u00c9 NIVEAU MAGN\u00c9TO-ORIGINEL.", "id": "Disebut level medan magnetik monster.", "is_bold": false, "pt": "CHAMADO DE N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL.", "text": "IT\u0027S CALLED THE PRIMAL MAGNETIC LEVEL.", "tr": "Buna \u0130lkel Odak Manyetik Seviyesi denir.", "type": "inside"}, {"angle": 0, "bbox": ["21", "440", "407", "638"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "LE NIVEAU MAGN\u00c9TO-ORIGINEL EST INOFFENSIF POUR LES \u00caTRES VIVANTS, MAIS IL PEUT AFFECTER LES \u00c9QUIPEMENTS \u00c9LECTRONIQUES.", "id": "Level medan magnetik tidak berbahaya bagi makhluk hidup, tapi bisa memengaruhi peralatan elektronik.", "is_bold": false, "pt": "O N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL \u00c9 INOFENSIVO PARA SERES VIVOS, MAS PODE AFETAR EQUIPAMENTOS ELETR\u00d4NICOS.", "text": "THE PRIMAL MAGNETIC LEVEL IS HARMLESS TO LIVING BEINGS BUT CAN AFFECT ELECTRONIC DEVICES.", "tr": "\u0130lkel Manyetik Seviye biyolojik varl\u0131klara zarars\u0131zd\u0131r, ancak elektronik cihazlar\u0131 etkileyebilir.", "type": "inside"}, {"angle": 0, "bbox": ["449", "440", "674", "616"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "LE NIVEAU MAGN\u00c9TIQUE DE CETTE B\u00caTE ORIGINELLE A D\u00c9J\u00c0 PERTURB\u00c9 L\u0027ENREGISTREMENT.", "id": "Level magnetik monster ini sudah mengganggu rekaman.", "is_bold": false, "pt": "O N\u00cdVEL MAGN\u00c9TICO DESTA BESTA PRIMORDIAL J\u00c1 INTERFERIU NA FILMAGEM.", "text": "THIS PRIMAL BEAST\u0027S MAGNETIC LEVEL INTERFERED WITH THE RECORDING.", "tr": "Bu \u0130lkel Canavar\u0131n manyetik seviyesi \u015fimdiden \u00e7ekimi etkiliyor.", "type": "inside"}, {"angle": 0, "bbox": ["835", "736", "1058", "960"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "EST-CE QUE PLUS LE NIVEAU MAGN\u00c9TO-ORIGINEL EST \u00c9LEV\u00c9, PLUS LA B\u00caTE ORIGINELLE EST PUISSANTE !?", "id": "Apakah semakin kuat level medan magnetiknya, semakin hebat monsternya!?", "is_bold": false, "pt": "QUANTO MAIS FORTE O N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL, MAIS PODEROSA \u00c9 A BESTA PRIMORDIAL, CERTO!?", "text": "DOES THAT MEAN THE STRONGER THE PRIMAL MAGNETIC LEVEL, THE STRONGER THE PRIMAL BEAST!?", "tr": "\u0130lkel Manyetik Seviye ne kadar g\u00fc\u00e7l\u00fcyse, \u0130lkel Canavar da o kadar m\u0131 g\u00fc\u00e7l\u00fc olur!?", "type": "inside"}, {"angle": -9.127498520698225, "bbox": ["257", "726", "328", "785"], "bg_color": ["215", "216", "216"], "fg_color": ["119", "119", "120"], "fr": "[SFX] BZZT", "id": "[SFX] ZZZT", "is_bold": false, "pt": "[SFX] BZZT", "text": "ZZZT", "tr": "[SFX] V\u0131zzz", "type": "sfx"}], "width": 1080}, {"height": 2225, "img_url": "snowmtl.ru/latest/the-original/205/10.webp", "translations": [{"angle": 0, "bbox": ["21", "97", "220", "281"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "NOUS UTILISONS LA FORCE DU NIVEAU MAGN\u00c9TO-ORIGINEL...", "id": "Kita menggunakan kuat lemahnya level medan magnetik", "is_bold": false, "pt": "N\u00d3S USAMOS A FOR\u00c7A DO N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL...", "text": "WE USE THE STRENGTH OF THE PRIMAL MAGNETIC LEVEL...", "tr": "Biz \u0130lkel Manyetik Seviyenin g\u00fcc\u00fcne g\u00f6re", "type": "inside"}, {"angle": 0, "bbox": ["114", "303", "326", "484"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "...POUR JUGER DE LA PUISSANCE DE COMBAT D\u0027UNE B\u00caTE ORIGINELLE OU...", "id": "Untuk menilai monster atau", "is_bold": false, "pt": "...PARA JULGAR O PODER DE COMBATE DE UMA BESTA PRIMORDIAL OU...", "text": "...TO DETERMINE A PRIMAL BEAST\u0027S OR...", "tr": "\u0130lkel Canavar\u0131n veya", "type": "inside"}, {"angle": 0, "bbox": ["841", "97", "1058", "267"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "...D\u0027UN VARIANT ORIGINEL !", "id": "Kekuatan tempur mutan!", "is_bold": false, "pt": "...DE UM METAMORFO PRIMORDIAL!", "text": "...A PRIMORDIAL VARIANT\u0027S COMBAT POWER!", "tr": "\u0130lkel Varyant\u0131n sava\u015f g\u00fcc\u00fcn\u00fc yarg\u0131lar\u0131z!", "type": "inside"}, {"angle": 0, "bbox": ["36", "841", "890", "1029"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "CONCERNANT LE NIVEAU MAGN\u00c9TO-ORIGINEL : LE PROTOTYPE DU NIVEAU MAGN\u00c9TO-ORIGINEL PROVIENT D\u0027UN PH\u00c9NOM\u00c8NE R\u00c9EL APPEL\u00c9 RAYONS COSMIQUES. POUR COMPRENDRE LE NIVEAU MAGN\u00c9TO-ORIGINEL, IL FAUT D\u0027ABORD COMPRENDRE LES RAYONS COSMIQUES. MAIS QUE SONT LES RAYONS COSMIQUES ? JE SUIS S\u00dbR QUE TOUT LE MONDE EST TR\u00c8S, TR\u00c8S IMPATIENT DE LE SAVOIR, ALORS LAISSEZ-MOI VOUS EN PARLER UN PEU ~", "id": "Mengenai level medan magnetik monster, prototipenya berasal dari sesuatu di dunia nyata yang disebut sinar kosmik. Untuk memahami level medan magnetik monster, kita perlu memahami sinar kosmik terlebih dahulu. Tapi apa itu sinar kosmik? Saya yakin semua orang sangat, sangat ingin tahu, jadi akan saya jelaskan~", "is_bold": false, "pt": "SOBRE O N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL: O PROT\u00d3TIPO DO N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL VEM DE ALGO NO MUNDO REAL CHAMADO RAIO C\u00d3SMICO. PARA ENTENDER O N\u00cdVEL MAGN\u00c9TICO PRIMORDIAL, \u00c9 PRECISO PRIMEIRO ENTENDER OS RAIOS C\u00d3SMICOS. MAS O QUE S\u00c3O RAIOS C\u00d3SMICOS? ACREDITO QUE TODOS EST\u00c3O MUITO ANSIOSOS PARA SABER, ENT\u00c3O VOU EXPLICAR PARA VOC\u00caS~", "text": "REGARDING THE PRIMAL MAGNETIC LEVEL:\nTHE PROTOTYPE FOR THE PRIMAL MAGNETIC LEVEL COMES FROM SOMETHING IN REALITY CALLED COSMIC RAYS.\nTO UNDERSTAND THE PRIMAL MAGNETIC LEVEL, ONE MUST FIRST UNDERSTAND COSMIC RAYS.\nBUT WHAT ARE COSMIC RAYS?\nI BELIEVE EVERYONE IS VERY EAGER TO KNOW, SO LET ME EXPLAIN~", "tr": "\u0130lkel Odak Manyetik Seviyesi Hakk\u0131nda: \u0130lkel Odak Manyetik Seviyesinin prototipi ger\u00e7ek d\u00fcnyada kozmik \u0131\u015f\u0131nlar olarak adland\u0131r\u0131lan bir \u015feyden gelir. \u0130lkel Odak Manyetik Seviyesini anlamak i\u00e7in \u00f6nce kozmik \u0131\u015f\u0131nlar\u0131 anlamak gerekir. Peki kozmik \u0131\u015f\u0131nlar nedir? Herkesin bunu \u00e7ok merak etti\u011fine eminim, o y\u00fczden size biraz anlatay\u0131m~", "type": "inside"}, {"angle": 0.0008578872911186863, "bbox": ["-8", "1968", "1088", "2077"], "bg_color": ["193", "193", "193"], "fg_color": ["163", "163", "163"], "fr": "...A UN IMPACT MAJEUR SUR LA CONCEPTION. COMPOSITION : L\u0027\u00c9LECTRICIT\u00c9 DANS L\u0027ATMOSPH\u00c8RE DE HENRY (IONISATION DE L\u0027ATMOSPH\u00c8RE TERRESTRE) PROVIENT UNIQUEMENT DE SUBSTANCES RADIOACTIVES DANS LE SOL OU DES RADIATIONS \u00c9MISES. DE 1900 \u00c0 1910, SUR UNE P\u00c9RIODE DE DIX ANS, LA MESURE DU TAUX D\u0027IONISATION \u00c0 DES ALTITUDES CROISSANTES...", "id": "Memiliki pengaruh besar dalam desain. Komponen: Arus listrik di atmosfer Henry (ionisasi lapisan atmosfer Bumi) hanya berasal dari zat radioaktif di tanah atau radiasi yang dihasilkan. Dari tahun 1900 hingga 1910, pengukuran laju ionisasi pada ketinggian yang meningkat secara bertahap dalam sepuluh tahun.", "is_bold": false, "pt": "TEM UM IMPACTO SIGNIFICATIVO NO DESIGN. COMPONENTES: A CORRENTE NA ATMOSFERA (IONIZA\u00c7\u00c3O DA ATMOSFERA TERRESTRE) INICIALMENTE SE ACREDITAVA VIR APENAS DE SUBST\u00c2NCIAS RADIOATIVAS NO SOLO OU DA RADIA\u00c7\u00c3O EMITIDA. ENTRE 1900 E 1910, MEDI\u00c7\u00d5ES DA TAXA DE IONIZA\u00c7\u00c3O EM ALTITUDES CRESCENTES AO LONGO DE DEZ ANOS...", "text": "IT HAS A SIGNIFICANT IMPACT ON DESIGN.\nCOMPOSITION:\nATMOSPHERIC CURRENT (IONIZATION OF EARTH\u0027S ATMOSPHERE) ORIGINATES ONLY FROM RADIOACTIVE SUBSTANCES IN THE SOIL OR THEIR EMITTED RADIATION.\nFROM 1900 TO 1910, MEASUREMENTS OVER THE DECADE SHOWED THE IONIZATION RATE INCREASING WITH ALTITUDE.", "tr": "Tasar\u0131m \u00fczerinde \u00f6nemli bir etkisi vard\u0131r. Bile\u015fenler: Henry, atmosferdeki ak\u0131m\u0131n (D\u00fcnya atmosferinin iyonla\u015fmas\u0131) yaln\u0131zca topraktaki radyoaktif maddelerden veya yay\u0131lan radyasyondan kaynakland\u0131\u011f\u0131n\u0131 [belirtti]. 1900-1910 y\u0131llar\u0131 aras\u0131nda, on y\u0131l i\u00e7inde artan y\u00fcksekliklerde iyonla\u015fma oran\u0131 \u00f6l\u00e7\u00fcld\u00fc.", "type": "outside"}, {"angle": -0.002354889019471784, "bbox": ["-54", "1330", "1116", "1404"], "bg_color": ["221", "221", "221"], "fg_color": ["133", "133", "133"], "fr": "LES RAYONS COSMIQUES, \u00c9GALEMENT APPEL\u00c9S RADIATIONS COSMIQUES, SONT DES PARTICULES SUBATOMIQUES CHARG\u00c9ES DE HAUTE \u00c9NERGIE PROVENANT DE L\u0027ESPACE EXTRA-ATMOSPH\u00c9RIQUE. ILS PEUVENT PRODUIRE DES PARTICULES SECONDAIRES QUI P\u00c9N\u00c8TRENT L\u0027ATMOSPH\u00c8RE ET LA SURFACE DE LA TERRE. LE TERME \"RAYON\" PROVIENT DU FAIT QU\u0027ILS \u00c9TAIENT AUTREFOIS CONSID\u00c9R\u00c9S COMME...", "id": "Sinar kosmik, juga dikenal sebagai radiasi kosmik, adalah partikel subatom berenergi tinggi yang bermuatan dari luar angkasa. Mereka dapat menghasilkan partikel sekunder yang menembus atmosfer dan permukaan Bumi. Istilah \u0027sinar\u0027 berasal dari anggapan historis bahwa mereka adalah", "is_bold": false, "pt": "OS RAIOS C\u00d3SMICOS, TAMB\u00c9M CONHECIDOS COMO RADIA\u00c7\u00c3O C\u00d3SMICA, S\u00c3O PART\u00cdCULAS SUBAT\u00d4MICAS CARREGADAS DE ALTA ENERGIA PROVENIENTES DO ESPA\u00c7O SIDERAL. ELES PODEM GERAR PART\u00cdCULAS SECUND\u00c1RIAS QUE PENETRAM A ATMOSFERA E A SUPERF\u00cdCIE DA TERRA. O TERMO \"RAIO\" ORIGINA-SE DO FATO DE QUE HISTORICAMENTE ERAM CONSIDERADOS...", "text": "Cosmic rays are high-energy charged subatomic particles originating from outer space. They can produce secondary particles that penetrate Earth\u0027s atmosphere and surface. The term \u0027ray\u0027 originates from their historical perception as electromagnetic radiation.", "tr": "Kozmik \u00e7izgiler, ayn\u0131 zamanda kozmik \u0131\u015f\u0131nlar olarak da bilinir, d\u0131\u015f uzaydan gelen y\u00fckl\u00fc, y\u00fcksek enerjili atom alt\u0131 par\u00e7ac\u0131klard\u0131r. D\u00fcnya\u0027n\u0131n atmosferine ve y\u00fczeyine n\u00fcfuz eden ikincil par\u00e7ac\u0131klar \u00fcretebilirler. I\u015f\u0131n terimi, bir zamanlar...", "type": "outside"}, {"angle": -0.07142425949899689, "bbox": ["-34", "1405", "1082", "1442"], "bg_color": ["193", "193", "193"], "fg_color": ["186", "186", "186"], "fr": "...UN RAYONNEMENT \u00c9LECTROMAGN\u00c9TIQUE. LES PRINCIPAUX RAYONS COSMIQUES PRIMAIRES (PARTICULES PROVENANT DE L\u0027ESPACE LOINTAIN ET ENTRANT EN COLLISION AVEC L\u0027ATMOSPH\u00c8RE)...", "id": "radiasi elektromagnetik. Sinar kosmik primer utama (partikel dari luar angkasa yang bertabrakan dengan atmosfer)", "is_bold": false, "pt": "...RADIA\u00c7\u00c3O ELETROMAGN\u00c9TICA. OS PRINCIPAIS RAIOS C\u00d3SMICOS PRIM\u00c1RIOS (PART\u00cdCULAS DO ESPA\u00c7O PROFUNDO QUE COLIDEM COM A ATMOSFERA)...", "text": "Primary cosmic rays (particles from deep space that collide with the atmosphere)", "tr": "...elektromanyetik radyasyon oldu\u011funun san\u0131ld\u0131\u011f\u0131 tarihsel bir yan\u0131lg\u0131dan kaynaklan\u0131r. Ana birincil kozmik \u0131\u015f\u0131nlar (derin uzaydan gelip atmosferle \u00e7arp\u0131\u015fan par\u00e7ac\u0131klar)...", "type": "outside"}, {"angle": 0, "bbox": ["-58", "1444", "1125", "1554"], "bg_color": ["225", "225", "225"], "fg_color": ["130", "130", "130"], "fr": "...SONT G\u00c9N\u00c9RALEMENT DES PARTICULES STABLES SUR TERRE, COMME LES PROTONS, LES NOYAUX ATOMIQUES OU LES \u00c9LECTRONS. CEPENDANT, UNE PROPORTION NON N\u00c9GLIGEABLE EST CONSTITU\u00c9E DE PARTICULES D\u0027ANTIMATI\u00c8RE STABLES, COMME LES POSITRONS OU LES ANTIPROTONS. CETTE PETITE FRACTION RESTANTE CONCERNE LES NOYAUX D\u0027H\u00c9LIUM (C\u0027EST-\u00c0-DIRE LES PARTICULES ALPHA)...", "id": "komponennya di Bumi umumnya adalah partikel stabil, seperti proton, inti atom, atau elektron. Namun, ada proporsi yang tidak kecil berupa partikel antimateri stabil, seperti positron atau antiproton. Bagian kecil yang tersisa ini adalah penelitian inti helium (yaitu partikel", "is_bold": false, "pt": "...S\u00c3O GERALMENTE PART\u00cdCULAS EST\u00c1VEIS NA TERRA, COMO PR\u00d3TONS, N\u00daCLEOS AT\u00d4MICOS OU EL\u00c9TRONS. NO ENTANTO, UMA PEQUENA PROPOR\u00c7\u00c3O CONSISTE EM PART\u00cdCULAS EST\u00c1VEIS DE ANTIMAT\u00c9RIA, COMO P\u00d3SITRONS OU ANTIPR\u00d3TONS. ESTA PEQUENA PARTE RESTANTE, INCLUINDO N\u00daCLEOS DE H\u00c9LIO (OU SEJA, PART\u00cdCULAS ALFA)...", "text": "on Earth are generally composed of stable particles, such as protons, atomic nuclei, or electrons. However, a very small proportion consists of stable antimatter particles, like positrons or anti-protons. This remaining small fraction is an active area of research.", "tr": "...bile\u015fenleri D\u00fcnya\u0027da genellikle protonlar, atom \u00e7ekirdekleri veya elektronlar gibi kararl\u0131 par\u00e7ac\u0131klard\u0131r. Ancak, pozitronlar veya antiprotonlar gibi kararl\u0131 antimadde par\u00e7ac\u0131klar\u0131ndan olu\u015fan az\u0131msanmayacak bir oran da vard\u0131r; bu geri kalan k\u00fc\u00e7\u00fck k\u0131s\u0131m, Helyum atom \u00e7ekirdeklerini inceler (yani par\u00e7ac\u0131klar...", "type": "outside"}, {"angle": -0.07473915347503635, "bbox": ["-17", "1516", "787", "1555"], "bg_color": ["195", "195", "195"], "fg_color": ["187", "187", "187"], "fr": "...UN DOMAINE DE RECHERCHE ACTIF. ENVIRON 89 % DES RAYONS COSMIQUES SONT DE SIMPLES PROTONS, 10 % SONT...", "id": "bidang penelitian aktif. Sekitar 89% sinar kosmik adalah proton murni, 10% adalah", "is_bold": false, "pt": "...\u00c9 UMA \u00c1REA DE PESQUISA ATIVA. APROXIMADAMENTE 89% DOS RAIOS C\u00d3SMICOS S\u00c3O SIMPLESMENTE PR\u00d3TONS, 10% S\u00c3O N\u00daCLEOS DE H\u00c9LIO (PART\u00cdCULAS ALFA),", "text": "Approximately 89% of cosmic rays are simple protons, 10% are helium nuclei (i.e., alpha particles),", "tr": "...man\u0131n aktif bir alan\u0131d\u0131r. Kozmik \u0131\u015f\u0131nlar\u0131n yakla\u015f\u0131k %89\u0027u salt protonlard\u0131r, %10\u0027u ise...", "type": "outside"}, {"angle": -0.04279698799987841, "bbox": ["5", "1556", "1076", "1592"], "bg_color": ["189", "189", "189"], "fg_color": ["197", "197", "197"], "fr": "...ET 1 % SONT DES \u00c9L\u00c9MENTS LOURDS. CES NOYAUX ATOMIQUES CONSTITUENT 99 % DES RAYONS COSMIQUES. LES \u00c9LECTRONS ISOL\u00c9S (COMME LES PARTICULES B\u00caTA)...", "id": "dan 1% sisanya adalah unsur berat. Inti atom ini membentuk 99% dari sinar kosmik. Elektron tunggal (seperti partikel", "is_bold": false, "pt": "E 1% S\u00c3O ELEMENTOS PESADOS. ESSES N\u00daCLEOS AT\u00d4MICOS CONSTITUEM 99% DOS RAIOS C\u00d3SMICOS. EL\u00c9TRONS SOLIT\u00c1RIOS (COMO PART\u00cdCULAS BETA)...", "text": "and 1% are heavy elements. These atomic nuclei constitute 99% of cosmic rays. Solitary electrons (such as particles,", "tr": "...Helyum atom \u00e7ekirdekleri ve %1\u0027i a\u011f\u0131r elementlerdir. Bu atom \u00e7ekirdekleri kozmik \u0131\u015f\u0131nlar\u0131n %99\u0027unu olu\u015fturur. Yaln\u0131z elektronlar (beta par\u00e7ac\u0131klar\u0131 gibi...", "type": "outside"}, {"angle": -0.02682652140649111, "bbox": ["-20", "1594", "458", "1668"], "bg_color": ["198", "198", "198"], "fg_color": ["153", "153", "153"], "fr": "...(BIEN QUE LEUR ORIGINE RESTE INCERTAINE) CONSTITUENT LA MAJEURE PARTIE DU 1 % RESTANT ;", "id": "meskipun sumbernya masih belum jelas) merupakan sisa 1% dan sebagian kecilnya.", "is_bold": false, "pt": "...(EMBORA SUA ORIGEM AINDA N\u00c3O SEJA CLARA) CONSTITUEM O 1% RESTANTE E UMA PEQUENA FRA\u00c7\u00c3O...", "text": "though their source remains unclear) make up the vast majority of the remaining 1%; gamma rays and ultra-high-energy neutrinos only account for", "tr": "...kayna\u011f\u0131 hala belirsiz olsa da) geri kalan %1\u0027lik ve daha k\u00fc\u00e7\u00fck bir k\u0131sm\u0131 olu\u015fturur;", "type": "outside"}, {"angle": -0.003555347368120465, "bbox": ["194", "1594", "1090", "1667"], "bg_color": ["218", "218", "218"], "fg_color": ["131", "131", "131"], "fr": "LES RAYONS GAMMA ET LES NEUTRINOS DE TR\u00c8S HAUTE \u00c9NERGIE N\u0027EN SONT QU\u0027UNE FAIBLE PROPORTION. LA DIVERSIT\u00c9 DES \u00c9NERGIES DES PARTICULES MONTRE QUE LES RAYONS COSMIQUES ONT DES SOURCES VARI\u00c9ES.", "id": "sebagian besar darinya; sinar gamma dan neutrino berenergi sangat tinggi hanya menyumbang sebagian kecil. Keanekaragaman energi partikel menunjukkan bahwa sinar kosmik memiliki sumber yang luas. Partikel-partikel ini", "is_bold": false, "pt": "...DA MAIOR PARTE; RAIOS GAMA E NEUTRINOS DE ENERGIA ULTRA-ALTA REPRESENTAM APENAS UMA PARTE. A DIVERSIFICA\u00c7\u00c3O DA ENERGIA DAS PART\u00cdCULAS MOSTRA QUE OS RAIOS C\u00d3SMICOS T\u00caM UMA AMPLA GAMA DE ORIGENS. DESTAS PART\u00cdCULAS...", "text": "a small fraction. The diversity in particle energies indicates that cosmic rays have a wide range of sources.", "tr": "b\u00fcy\u00fck \u00e7o\u011funlu\u011funu; Gama \u0131\u015f\u0131nlar\u0131 ve ultra y\u00fcksek enerjili n\u00f6trinolar ise yaln\u0131zca k\u00fc\u00e7\u00fck bir pay tutar. Par\u00e7ac\u0131k enerjilerinin \u00e7e\u015fitlili\u011fi, kozmik \u0131\u015f\u0131nlar\u0131n geni\u015f bir kaynak yelpazesine sahip oldu\u011funu g\u00f6sterir. Bu par\u00e7ac\u0131klar\u0131n...", "type": "outside"}, {"angle": -0.02697173984802248, "bbox": ["57", "1632", "220", "1666"], "bg_color": ["199", "199", "199"], "fg_color": ["189", "189", "189"], "fr": "DE CES PARTICULES... UNE PARTIE.", "id": "adalah bagian darinya.", "is_bold": false, "pt": "...UMA PARTE.", "text": "of a part.", "tr": "bir k\u0131sm\u0131d\u0131r.", "type": "outside"}, {"angle": -0.06115309989192497, "bbox": ["-13", "1668", "1076", "1704"], "bg_color": ["191", "191", "191"], "fg_color": ["193", "193", "193"], "fr": "LEUR ORIGINE PEUT \u00caTRE LE SOLEIL (OU D\u0027AUTRES \u00c9TOILES) OU L\u0027UNIVERS VISIBLE LOINTAIN, PRODUITS PAR DES M\u00c9CANISMES PHYSIQUES ENCORE INCONNUS.", "id": "Sumbernya mungkin Matahari (atau bintang lain) atau dari alam semesta kasatmata yang jauh, dihasilkan oleh beberapa mekanisme fisika yang belum diketahui.", "is_bold": false, "pt": "A ORIGEM PODE SER O SOL (OU OUTRAS ESTRELAS) OU DO UNIVERSO VIS\u00cdVEL DISTANTE, PRODUZIDOS POR ALGUNS MECANISMOS F\u00cdSICOS AINDA DESCONHECIDOS.", "text": "The sources of these particles might be the Sun (or other stars) or originate from the distant observable universe, produced by some yet unknown physical mechanisms.", "tr": "kaynaklar\u0131 G\u00fcne\u015f (veya di\u011fer y\u0131ld\u0131zlar) olabilir veya baz\u0131 hen\u00fcz bilinmeyen fiziksel...", "type": "outside"}, {"angle": -0.029275165353567445, "bbox": ["-57", "1705", "1132", "1817"], "bg_color": ["226", "226", "226"], "fg_color": ["131", "131", "131"], "fr": "LES RAYONS COSMIQUES PEUVENT AVOIR DES \u00c9NERGIES D\u00c9PASSANT 10^20 EV, BIEN AU-DEL\u00c0 DES 10^12 \u00c0 10^13 EV ATTEIGNABLES PAR LES ACC\u00c9L\u00c9RATEURS DE PARTICULES SUR TERRE, CE QUI SUSCITE UN GRAND INT\u00c9R\u00caT POUR L\u0027\u00c9TUDE DES RAYONS COSMIQUES DE PLUS HAUTE \u00c9NERGIE.", "id": "mekanisme tersebut. Energi sinar kosmik dapat melebihi 10^20 eV, jauh melampaui 10^12 hingga 10^13 eV yang dapat dicapai oleh akselerator partikel di Bumi, membuat banyak orang tertarik untuk meneliti sinar kosmik berenergi lebih tinggi.", "is_bold": false, "pt": "A ENERGIA DOS RAIOS C\u00d3SMICOS PODE EXCEDER 10^20 EV, MUITO AL\u00c9M DOS 10^12 A 10^13 EV ATING\u00cdVEIS PELOS ACELERADORES DE PART\u00cdCULAS NA TERRA, O QUE FAZ COM QUE MUITAS PESSOAS SE INTERESSEM E PESQUISEM RAIOS C\u00d3SMICOS DE MAIOR ENERGIA.", "text": "The energy of cosmic rays can exceed 10^20 eV, far surpassing the 10^12 to 10^13 eV achievable by particle accelerators on Earth, making cosmic rays with even greater energies a subject of intense interest and research.", "tr": "...mekanizmalar taraf\u0131ndan \u00fcretilmi\u015f olabilir. Kozmik \u0131\u015f\u0131nlar\u0131n enerjisi 10^20 eV\u0027yi a\u015fabilir, bu da D\u00fcnya\u0027daki par\u00e7ac\u0131k h\u0131zland\u0131r\u0131c\u0131lar\u0131n ula\u015fabilece\u011fi 10^12 ila 10^13 eV\u0027nin \u00e7ok \u00fczerindedir, bu da bir\u00e7ok insan\u0131n daha y\u00fcksek enerjili kozmik \u0131\u015f\u0131nlara ilgi duymas\u0131na ve ara\u015ft\u0131rmaya y\u00f6nelmesine neden olmu\u015ftur.", "type": "outside"}, {"angle": 3.0125823088930742e-06, "bbox": ["203", "1781", "893", "1817"], "bg_color": ["190", "190", "190"], "fg_color": ["216", "216", "216"], "fr": "PAR LE PROCESSUS DE NUCL\u00c9OSYNTH\u00c8SE DES RAYONS COSMIQUES, CEUX-CI JOUENT UN R\u00d4LE MAJEUR DANS LA PRODUCTION DE LITHIUM,", "id": "Melalui proses nukleosintesis sinar kosmik, sinar kosmik berperan penting dalam", "is_bold": false, "pt": "ATRAV\u00c9S DO PROCESSO DE NUCLEOSS\u00cdNTESE POR RAIOS C\u00d3SMICOS, OS RAIOS C\u00d3SMICOS DESEMPENHAM UM PAPEL IMPORTANTE NA PRODU\u00c7\u00c3O DE L\u00cdTIO, BER\u00cdLIO E BORO NO UNIVERSO.", "text": "Through the process of cosmic ray nucleosynthesis, cosmic rays play a major role in the cosmic abundance of Lithium,", "tr": "Kozmik \u0131\u015f\u0131n n\u00fckleosentezi s\u00fcreciyle, kozmik \u0131\u015f\u0131nlar evrendeki Lityum,", "type": "outside"}, {"angle": -0.0004849498536430019, "bbox": ["893", "1781", "1050", "1817"], "bg_color": ["186", "186", "186"], "fg_color": ["217", "217", "217"], "fr": "...DE B\u00c9RYLLIUM ET DE BORE DANS L\u0027UNIVERS.", "id": "pembentukan litium, berilium, dan boron di alam semesta.", "is_bold": false, "pt": "BER\u00cdLIO E BORO", "text": "Beryllium, and Boron.", "tr": "Berilyum ve Bor\u0027un", "type": "outside"}, {"angle": -0.05739601067327271, "bbox": ["-9", "1818", "1034", "1853"], "bg_color": ["190", "190", "190"], "fg_color": ["203", "203", "203"], "fr": "ILS PRODUISENT \u00c9GALEMENT CERTAINS ISOTOPES RADIOACTIFS SUR TERRE, TELS QUE...", "id": "Mereka juga menghasilkan beberapa isotop radioaktif di Bumi, seperti", "is_bold": false, "pt": "ELES TAMB\u00c9M PRODUZEM ALGUNS IS\u00d3TOPOS RADIOATIVOS NA TERRA, COMO O CARBONO-14.", "text": "They also produce some radioactive isotopes on Earth, such as", "tr": "olu\u015fumunda \u00f6nemli bir rol oynar. Ayr\u0131ca D\u00fcnya\u0027da baz\u0131 radyoaktif izotoplar da \u00fcretirler, \u00f6rne\u011fin", "type": "outside"}, {"angle": -0.0427106829913555, "bbox": ["-63", "1855", "1118", "1965"], "bg_color": ["223", "223", "223"], "fg_color": ["131", "131", "131"], "fr": "...LE CARBONE 14. DANS L\u0027HISTOIRE DE LA PHYSIQUE DES PARTICULES, LES RAYONS COSMIQUES SONT RESPONSABLES D\u0027UNE GRANDE PARTIE DU RAYONNEMENT DE FOND SUR TERRE. COMME LES RAYONS COSMIQUES SONT TR\u00c8S INTENSES EN DEHORS DE L\u0027ATMOSPH\u00c8RE TERRESTRE ET DANS LES CHAMPS MAGN\u00c9TIQUES, ASSURER LA S\u00c9CURIT\u00c9 DES ASTRONAUTES \u00c0 BORD DES VAISSEAUX SPATIAUX VOYAGEANT DANS L\u0027ESPACE INTERPLAN\u00c9TAIRE...", "id": "karbon-14. Dalam sejarah fisika partikel, sinar kosmik juga menyebabkan sebagian besar radiasi latar di Bumi. Karena sinar kosmik di luar atmosfer dan medan magnet Bumi sangat kuat, maka untuk menjaga keselamatan astronaut di pesawat ruang angkasa yang melakukan perjalanan di ruang antarplanet,", "is_bold": false, "pt": "NA HIST\u00d3RIA DA F\u00cdSICA DE PART\u00cdCULAS, OS RAIOS C\u00d3SMICOS TAMB\u00c9M CAUSARAM UMA GRANDE PARTE DA RADIA\u00c7\u00c3O DE FUNDO NA TERRA. COMO OS RAIOS C\u00d3SMICOS FORA DA ATMOSFERA E DO CAMPO MAGN\u00c9TICO DA TERRA S\u00c3O MUITO FORTES, ELES S\u00c3O UMA PREOCUPA\u00c7\u00c3O PARA A SEGURAN\u00c7A DOS ASTRONAUTAS EM NAVES ESPACIAIS QUE VIAJAM NO ESPA\u00c7O INTERPLANET\u00c1RIO.", "text": "Carbon-14. In the history of particle physics, cosmic rays also cause a large part of Earth\u0027s background radiation. Because cosmic rays outside Earth\u0027s atmosphere and magnetic field are very strong, therefore, for maintaining the safety of astronauts on spacecraft navigating interstellar space,", "tr": "Karbon-14. Par\u00e7ac\u0131k fizi\u011fi tarihinde, kozmik \u0131\u015f\u0131nlar ayr\u0131ca D\u00fcnya\u0027daki arka plan radyasyonunun b\u00fcy\u00fck bir k\u0131sm\u0131na neden olmu\u015ftur. D\u00fcnya atmosferinin d\u0131\u015f\u0131nda ve manyetik alanlardaki kozmik \u0131\u015f\u0131nlar \u00e7ok g\u00fc\u00e7l\u00fc oldu\u011fundan, gezegenler aras\u0131 uzayda seyahat eden uzay gemilerindeki astronotlar\u0131n g\u00fcvenli\u011fini sa\u011flamak i\u00e7in,", "type": "outside"}, {"angle": -0.07438812806248052, "bbox": ["410", "1855", "812", "1892"], "bg_color": ["195", "195", "195"], "fg_color": ["216", "216", "216"], "fr": "LE POSITRON,", "id": "positron,", "is_bold": false, "pt": "P\u00d3SITRONS, M\u00daONS E M\u00c9SIONS PI FORAM DESCOBERTOS NOS RAIOS C\u00d3SMICOS.", "text": "Positrons were discovered in cosmic rays,", "tr": "kozmik \u0131\u015f\u0131nlarda pozitronlar,", "type": "outside"}, {"angle": -0.07438812806233841, "bbox": ["840", "1855", "913", "1891"], "bg_color": ["198", "198", "198"], "fg_color": ["216", "216", "216"], "fr": "...LE MUON ET", "id": "muon, dan", "is_bold": false, "pt": "M\u00daONS E", "text": "muons and", "tr": "m\u00fconlar ve", "type": "outside"}, {"angle": -6.589071330154184e-05, "bbox": ["935", "1855", "1075", "1891"], "bg_color": ["207", "207", "207"], "fg_color": ["161", "161", "161"], "fr": "...LE PION ONT \u00c9T\u00c9 D\u00c9COUVERTS GR\u00c2CE AUX RAYONS COSMIQUES.", "id": "meson ditemukan dari sinar kosmik. Alam semesta", "is_bold": false, "pt": "M\u00c9SIONS.", "text": "mesons. Cos", "tr": "mezonlar ke\u015ffedildi. Kozmik...", "type": "outside"}, {"angle": -0.047802836343976196, "bbox": ["478", "1967", "1062", "2004"], "bg_color": ["193", "193", "193"], "fg_color": ["171", "171", "171"], "fr": "APR\u00c8S LA D\u00c9COUVERTE DE LA RADIOACTIVIT\u00c9 PAR BECQUEREL EN 1896, BEAUCOUP PENSAIENT...", "id": "Setelah Becquerel menemukan radioaktivitas pada tahun 1896, banyak orang percaya", "is_bold": false, "pt": "DEPOIS QUE BECQUEREL DESCOBRIU A RADIOATIVIDADE EM 1896, MUITOS ACREDITAVAM...", "text": "After Becquerel discovered radioactivity in 1896, many people believed", "tr": "Becquerel\u0027in 1896\u0027da radyoaktiviteyi ke\u015ffetmesinden sonra, bir\u00e7ok ki\u015fi,", "type": "outside"}, {"angle": -0.002354889032488927, "bbox": ["-13", "2042", "345", "2079"], "bg_color": ["198", "198", "198"], "fg_color": ["132", "132", "132"], "fr": "...QUE LES GAZ PRODUITS (ISOTOPES DU RADON)...", "id": "gas (isotop radon) yang dihasilkan", "is_bold": false, "pt": "...QUE GASES PRODUZIDOS (IS\u00d3TOPOS DE RAD\u00d4NIO)...", "text": "generated gas (isotopes of radon gas)", "tr": "\u00fcretilen gazlar\u0131n (radon gaz\u0131n\u0131n izotoplar\u0131)", "type": "outside"}, {"angle": -0.06794958686560904, "bbox": ["-38", "2079", "1005", "2115"], "bg_color": ["191", "191", "191"], "fg_color": ["205", "205", "205"], "fr": "...MONTRAIENT UNE DIMINUTION QUI POUVAIT S\u0027EXPLIQUER PAR L\u0027ABSORPTION DU RAYONNEMENT IONISANT PAR L\u0027AIR. PAR LA SUITE, VICTOR...", "id": "menunjukkan penurunan nilai yang dapat dijelaskan oleh penyerapan radiasi pengion oleh udara. Setelah itu, Victor", "is_bold": false, "pt": "...MOSTRARAM UMA DIMINUI\u00c7\u00c3O QUE PODERIA SER EXPLICADA PELA ABSOR\u00c7\u00c3O DA RADIA\u00c7\u00c3O IONIZANTE PELO AR. POSTERIORMENTE, VICTOR HESS...", "text": "showed a decrease that could be explained by the absorption of ionizing radiation by air. Afterwards, Victor", "tr": "iyonla\u015ft\u0131r\u0131c\u0131 radyasyonun hava taraf\u0131ndan emilmesiyle a\u00e7\u0131klanabilen bir azalma g\u00f6sterdi\u011fini d\u00fc\u015f\u00fcnd\u00fc. Daha sonra, Victor", "type": "outside"}, {"angle": -0.05865889659270351, "bbox": ["1022", "2079", "1061", "2114"], "bg_color": ["182", "182", "182"], "fg_color": ["202", "202", "202"], "fr": "...HESS,", "id": "Hess", "is_bold": false, "pt": "HESS", "text": "Hess", "tr": "Hess,", "type": "outside"}, {"angle": -0.01297901784286637, "bbox": ["-26", "2117", "1074", "2154"], "bg_color": ["195", "195", "195"], "fg_color": ["196", "196", "196"], "fr": "...EN 1912, UTILISA UN BALLON \u00c0 AIR CHAUD POUR EMPORTER TROIS \u00c9LECTROSCOPES \u00c0 UNE ALTITUDE DE 5300 M\u00c8TRES. IL D\u00c9TECTA...", "id": "pada tahun 1912, menggunakan balon udara panas, membawa tiga elektrometer, naik ke ketinggian 5300 meter. Dia mendeteksi", "is_bold": false, "pt": "...EM 1912, USANDO UM BAL\u00c3O DE AR QUENTE, LEVOU TR\u00caS ELETROSC\u00d3PIOS A UMA ALTITUDE DE 5300 METROS. ELE DETECTOU...", "text": "In 1912, using a hot air balloon, carrying three electrometers, ascended to an altitude of 5300 meters. He detected", "tr": "1912\u0027de bir s\u0131cak hava balonu kullanarak, \u00fc\u00e7 elektrometreyi 5300 metre y\u00fcksekli\u011fe \u00e7\u0131kard\u0131. \u015eunu tespit etti:", "type": "outside"}, {"angle": 0.0127015849077452, "bbox": ["-17", "2154", "1086", "2224"], "bg_color": ["228", "228", "228"], "fg_color": ["133", "133", "133"], "fr": "...QUE LE TAUX D\u0027IONISATION AUGMENTAIT JUSQU\u0027\u00c0 ENVIRON QUATRE FOIS CELUI AU SOL. IL CONCLUT : \"LA MEILLEURE EXPLICATION DE MES OBSERVATIONS EST QU\u0027UN RAYONNEMENT TR\u00c8S P\u00c9N\u00c9TRANT...\"", "id": "bahwa tingkat ionisasi meningkat sekitar empat kali lipat dari tingkat di darat. Kesimpulannya adalah, \u0027Penjelasan terbaik untuk hasil pengamatan saya adalah", "is_bold": false, "pt": "...QUE A TAXA DE IONIZA\u00c7\u00c3O AUMENTOU PARA CERCA DE QUATRO VEZES A TAXA AO N\u00cdVEL DO SOLO. SUA CONCLUS\u00c3O FOI: \"A MELHOR EXPLICA\u00c7\u00c3O PARA MINHAS OBSERVA\u00c7\u00d5ES...\"", "text": "that the ionization rate increased to about four times the rate at ground level. He concluded that \u0027the best explanation for my observations...", "tr": "iyonla\u015fma oran\u0131n\u0131n yer seviyesindekinin yakla\u015f\u0131k d\u00f6rt kat\u0131na \u00e7\u0131kt\u0131\u011f\u0131n\u0131. Vard\u0131\u011f\u0131 sonu\u00e7 \u015fuydu: \u0027G\u00f6zlemlerimin en iyi a\u00e7\u0131klamas\u0131...", "type": "outside"}, {"angle": -2.0255706829175324e-05, "bbox": ["-13", "2192", "406", "2215"], "bg_color": ["196", "196", "196"], "fg_color": ["174", "174", "174"], "fr": "...UN RAYONNEMENT TR\u00c8S P\u00c9N\u00c9TRANT VENANT D\u0027EN HAUT...", "id": "sejenis radiasi yang sangat kuat dan menembus", "is_bold": false, "pt": "\"...\u00c9 UMA RADIA\u00c7\u00c3O DE ALTA PENETRA\u00c7\u00c3O QUE ENTRA NA ATMOSFERA VINDA DE CIMA.\"", "text": "is a highly penetrating radiation originating from", "tr": "...yukar\u0131dan gelen bir t\u00fcr g\u00fc\u00e7l\u00fc n\u00fcfuz edici \u0131\u015f\u0131n\u0131n,", "type": "outside"}, {"angle": 0.07232547597372312, "bbox": ["487", "2192", "564", "2215"], "bg_color": ["199", "199", "199"], "fg_color": ["175", "175", "175"], "fr": "...P\u00c9N\u00c8TRE", "id": "memasuki", "is_bold": false, "pt": "ENTRANDO...", "text": "entering", "tr": "...atmosfere girmesidir.\u0027", "type": "outside"}, {"angle": 0.06322398130620556, "bbox": ["675", "2193", "810", "2216"], "bg_color": ["200", "200", "200"], "fg_color": ["0", "0", "0"], "fr": "...NOTRE ATMOSPH\u00c8RE.\" (VICTOR HESS)", "id": "atmosfer dari atas.\u0027", "is_bold": false, "pt": "\"", "text": " Victor Hess", "tr": "Victor", "type": "outside"}, {"angle": -5.638655392203873e-05, "bbox": ["820", "2192", "1039", "2215"], "bg_color": ["196", "196", "196"], "fg_color": ["167", "167", "167"], "fr": "HESS, POUR CETTE D\u00c9COUVERTE...", "id": "Hess, karena penemuan ini,", "is_bold": false, "pt": "...HESS, POR ESTA DESCOBERTA...", "text": "Hess, because of this", "tr": "Hess bu [ke\u015ffi] nedeniyle...", "type": "outside"}], "width": 1080}, {"height": 1650, "img_url": "snowmtl.ru/latest/the-original/205/11.webp", "translations": [{"angle": -5.159806221399776e-06, "bbox": ["4", "238", "1089", "436"], "bg_color": ["215", "215", "215"], "fg_color": ["132", "132", "132"], "fr": "L\u0027ORIGINE SE R\u00c9F\u00c8RE G\u00c9N\u00c9RALEMENT AU MOUVEMENT ET \u00c0 LA DISTRIBUTION DANS L\u0027ESPACE INTERSTELLAIRE DES PRINCIPAUX COMPOSANTS DES RAYONS COSMIQUES \u2013 DIVERS NOYAUX ATOMIQUES \u2013 CE QUI REL\u00c8VE DU PROBL\u00c8ME DE LA PROPAGATION DES RAYONS COSMIQUES. L\u0027ORIGINE ET LA PROPAGATION DES RAYONS COSMIQUES SONT \u00c9TROITEMENT LI\u00c9ES : LES PHASES D\u0027ACC\u00c9L\u00c9RATION ET DE PROPAGATION NE PEUVENT \u00caTRE CLAIREMENT S\u00c9PAR\u00c9ES. L\u0027ORIGINE D\u0027UNE PARTIE CONSID\u00c9RABLE DES NOYAUX DES RAYONS COSMIQUES PRIMAIRES EST UNE QUESTION IMPORTANTE. LES RAYONS COSMIQUES, EN TANT QUE PRODUITS DE DIVERS PROCESSUS ASTROPHYSIQUES DE HAUTE \u00c9NERGIE, TRANSPORTENT UNE RICHE INFORMATION SUR CES PROCESSUS. PREMI\u00c8REMENT, PARCE QUE LES PARTICULES CHARG\u00c9ES DES RAYONS COSMIQUES DANS L\u0027ESPACE INTERSTELLAIRE...", "id": "Sumber biasanya merujuk pada komponen utama sinar kosmik\u2014gerakan dan distribusi berbagai inti atom di ruang antarbintang, yang termasuk dalam masalah propagasi sinar kosmik. Asal usul dan propagasi sinar kosmik saling terkait erat: tahap percepatan dan propagasi tidak dapat dipisahkan secara tegas; sebagian besar inti atom sinar kosmik primer adalah masalah penting. Apakah sinar kosmik, khususnya produk dari berbagai proses astrofisika berenergi tinggi, membawa informasi yang kaya tentang proses ini? Pertama, karena partikel bermuatan sinar kosmik di ruang antarbintang", "is_bold": false, "pt": "A ORIGEM E PROPAGA\u00c7\u00c3O DOS RAIOS C\u00d3SMICOS: O MOVIMENTO E DISTRIBUI\u00c7\u00c3O DOS PRINCIPAIS COMPONENTES DOS RAIOS C\u00d3SMICOS \u2014 V\u00c1RIOS N\u00daCLEOS AT\u00d4MICOS \u2014 NO ESPA\u00c7O INTERESTELAR S\u00c3O QUEST\u00d5ES DE PROPAGA\u00c7\u00c3O. A ORIGEM E PROPAGA\u00c7\u00c3O DOS RAIOS C\u00d3SMICOS EST\u00c3O INTRINSECAMENTE LIGADAS: AS FASES DE ACELERA\u00c7\u00c3O E PROPAGA\u00c7\u00c3O N\u00c3O PODEM SER CLARAMENTE SEPARADAS. UMA QUEST\u00c3O IMPORTANTE \u00c9 SE OS RAIOS C\u00d3SMICOS, PARTICULARMENTE UMA PARTE SIGNIFICATIVA DOS N\u00daCLEOS PRIM\u00c1RIOS, S\u00c3O PRODUTOS DE V\u00c1RIOS PROCESSOS ASTROF\u00cdSICOS DE ALTA ENERGIA, CARREGANDO RICA INFORMA\u00c7\u00c3O SOBRE ESSES PROCESSOS. PRIMEIRO, DEVIDO \u00c0S PART\u00cdCULAS CARREGADAS DOS RAIOS C\u00d3SMICOS NO ESPA\u00c7O INTERESTELAR,", "text": "The source usually refers to the main components of cosmic rays\u2014various atomic nuclei\u2014their motion and distribution in space, which belongs to the problem of cosmic ray propagation. The origin and propagation of cosmic rays are related: the acceleration and propagation phases cannot be clearly separated; a considerable portion of primary cosmic ray atomic nuclei, is an important issue. Whether cosmic rays are products of various high-energy astrophysical processes, carrying rich information about these processes. Firstly, because cosmic ray charged particles in interstellar space", "tr": "\u00c7ekirdek kayna\u011f\u0131 genellikle kozmik \u0131\u015f\u0131nlar\u0131n ana bile\u015fenleri olan \u00e7e\u015fitli atom \u00e7ekirdeklerinin uzaydaki hareketini ve da\u011f\u0131l\u0131m\u0131n\u0131 ifade eder ve kozmik \u0131\u015f\u0131nlar\u0131n yay\u0131lma sorununa aittir. Kozmik \u0131\u015f\u0131nlar\u0131n k\u00f6keni ve yay\u0131l\u0131m\u0131 birbiriyle yak\u0131ndan ili\u015fkilidir: h\u0131zlanma ve yay\u0131lma a\u015famalar\u0131 net bir \u015fekilde ayr\u0131lamaz; birincil kozmik \u0131\u015f\u0131n atom \u00e7ekirdeklerinin \u00f6nemli bir k\u0131sm\u0131 \u00f6nemli bir sorundur. Kozmik \u0131\u015f\u0131nlar\u0131n, \u00f6zellikle \u00e7e\u015fitli y\u00fcksek enerjili astrofiziksel s\u00fcre\u00e7lerin \u00fcr\u00fcnleri olup olmad\u0131\u011f\u0131, bu s\u00fcre\u00e7lere dair zengin bilgiler ta\u015f\u0131y\u0131p ta\u015f\u0131mad\u0131\u011f\u0131, \u00f6ncelikle kozmik \u0131\u015f\u0131n y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131n\u0131n y\u0131ld\u0131zlararas\u0131 uzayda...", "type": "outside"}, {"angle": -0.07891157922799152, "bbox": ["11", "405", "598", "436"], "bg_color": ["213", "213", "213"], "fg_color": ["134", "134", "134"], "fr": "...SONT D\u00c9VI\u00c9ES PAR LES CHAMPS MAGN\u00c9TIQUES. CEPENDANT, L\u0027\u00c9TUDE DE L\u0027ORIGINE ET DE LA PROPAGATION DES RAYONS COSMIQUES PR\u00c9SENTE DE NOMBREUSES DIFFICULT\u00c9S :", "id": "informasi. Namun, penelitian tentang asal usul dan propagasi sinar kosmik memiliki banyak kesulitan:", "is_bold": false, "pt": "O ESTUDO DA ORIGEM E PROPAGA\u00c7\u00c3O DOS RAIOS C\u00d3SMICOS ENFRENTA MUITAS DIFICULDADES:", "text": "information. However, the study of cosmic ray origin and propagation faces many difficulties:", "tr": "...bulunmas\u0131ndan kaynaklanmaktad\u0131r. Ancak, kozmik \u0131\u015f\u0131nlar\u0131n k\u00f6keni ve yay\u0131l\u0131m\u0131n\u0131n ara\u015ft\u0131r\u0131lmas\u0131nda bir\u00e7ok zorluk vard\u0131r:", "type": "outside"}, {"angle": -0.0010002136481830348, "bbox": ["7", "1365", "354", "1396"], "bg_color": ["186", "186", "186"], "fg_color": ["151", "151", "151"], "fr": "...1. D\u00c9VIATION : LES PARTICULES CHARG\u00c9ES SE D\u00c9PLACENT DE MANI\u00c8RE AL\u00c9ATOIRE...", "id": "Mekanisme: Partikel bermuatan bergerak secara acak dengan", "is_bold": false, "pt": "RESTRI\u00c7\u00d5ES: PART\u00cdCULAS CARREGADAS EM MOVIMENTO ALEAT\u00d3RIO...", "text": "constraints: Charged particles undergo random motion", "tr": "K\u0131s\u0131tlamalar: Y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131n rastgele hareketleriyle birlikte,", "type": "outside"}, {"angle": -1.2912464784920985, "bbox": ["0", "1496", "1084", "1660"], "bg_color": ["223", "223", "223"], "fg_color": ["134", "134", "134"], "fr": "LES ONDES DE CHOC PLUS INTENSES PROVOQU\u00c9ES PAR DES ACTIVIT\u00c9S \u00c0 HAUTE \u00c9NERGIE TELLES QUE LES EXPLOSIONS DE SUPERNOVA PEUVENT SE PROPAGER SUR DES DISTANCES SUFFISANTES DANS LE GAZ CHAUD ET RAR\u00c9FI\u00c9 DE L\u0027ESPACE INTERSTELLAIRE, PERMETTANT AUX M\u00c9CANISMES D\u0027ACC\u00c9L\u00c9RATION PAR ONDE DE CHOC D\u0027ACC\u00c9L\u00c9RER EFFICACEMENT LES PARTICULES DES RAYONS COSMIQUES. CEPENDANT, ON A R\u00c9CEMMENT D\u00c9COUVERT QUE LA DISTRIBUTION DE L\u0027ABONDANCE DES \u00c9L\u00c9MENTS DANS LES RAYONS COSMIQUES PRIMORDIAUX EST \u00c9TROITEMENT LI\u00c9E \u00c0 LA PREMI\u00c8RE \u00c9NERGIE D\u0027IONISATION DES ATOMES : PLUS LA PREMI\u00c8RE \u00c9NERGIE D\u0027IONISATION D\u0027UN \u00c9L\u00c9MENT EST FAIBLE, PLUS SON ABONDANCE RELATIVE DANS LES RAYONS COSMIQUES PRIMORDIAUX EST \u00c9LEV\u00c9E. CELA SUGG\u00c8RE QUE LA TEMP\u00c9RATURE DANS LES R\u00c9GIONS D\u0027ORIGINE ET D\u0027ACC\u00c9L\u00c9RATION DES RAYONS COSMIQUES NE PEUT PAS \u00caTRE TROP \u00c9LEV\u00c9E (\u003c 10^4 K), CE QUI POSE DES PROBL\u00c8MES POUR LES MOD\u00c8LES DE SUPERNOVA...", "id": "Gelombang kejut yang lebih kuat yang disebabkan oleh aktivitas berenergi tinggi seperti ledakan supernova dapat merambat cukup jauh dalam gas panas dan renggang di ruang antarbintang, memungkinkan mekanisme percepatan gelombang kejut untuk mempercepat partikel sinar kosmik secara efektif. Namun, baru-baru ini ditemukan bahwa distribusi kelimpahan unsur sinar kosmik purba sangat terkait dengan energi ionisasi pertama atom: semakin rendah energi ionisasi pertama suatu unsur, kelimpahan sinar kosmik purba dan suhu daerah asal dan percepatan sinar kosmik tidak boleh terlalu tinggi (\u003c10^4 K), membuat supernova", "is_bold": false, "pt": "ONDAS DE CHOQUE MAIS FORTES CAUSADAS POR ATIVIDADES DE ALTA ENERGIA, COMO EXPLOS\u00d5ES DE SUPERNOVAS, PODEM SE PROPAGAR POR DIST\u00c2NCIAS SUFICIENTEMENTE LONGAS EM GASES QUENTES E RAREFEITOS NO ESPA\u00c7O INTERESTELAR, PERMITINDO QUE MECANISMOS DE ACELERA\u00c7\u00c3O POR ONDA DE CHOQUE ACELEREM EFICAZMENTE AS PART\u00cdCULAS DE RAIOS C\u00d3SMICOS. NO ENTANTO, DESCOBERTAS RECENTES MOSTRAM QUE A DISTRIBUI\u00c7\u00c3O DA ABUND\u00c2NCIA ELEMENTAR DOS RAIOS C\u00d3SMICOS PRIMITIVOS EST\u00c1 INTIMAMENTE RELACIONADA COM A PRIMEIRA ENERGIA DE IONIZA\u00c7\u00c3O AT\u00d4MICA: QUANTO MENOR A PRIMEIRA ENERGIA DE IONIZA\u00c7\u00c3O DE UM ELEMENTO, MAIOR SUA ABUND\u00c2NCIA NOS RAIOS C\u00d3SMICOS PRIMITIVOS. ISSO SUGERE QUE A TEMPERATURA DAS REGI\u00d5ES DE ORIGEM E ACELERA\u00c7\u00c3O DOS RAIOS C\u00d3SMICOS N\u00c3O PODE SER MUITO ALTA (\u003c 10^4 K), O QUE IMPLICA RESTRI\u00c7\u00d5ES AOS MODELOS DE SUPERNOVA...", "text": "Stronger shock waves caused by high-energy events like supernova explosions can travel long distances in the hot, thin gas of interstellar space, potentially allowing shock wave acceleration mechanisms to effectively accelerate cosmic ray particles. However, recent findings show a close correlation between the abundance distribution of primary cosmic ray elements and their first ionization energy: elements with lower first ionization energy suggest that the temperature in the origin and acceleration regions of cosmic rays cannot be too high (\u003c 10^4 K), which implies that supernova...", "tr": "S\u00fcpernova patlamalar\u0131 gibi y\u00fcksek enerjili olaylar\u0131n neden oldu\u011fu daha g\u00fc\u00e7l\u00fc \u015fok dalgalar\u0131, y\u0131ld\u0131zlararas\u0131 uzaydaki y\u00fcksek s\u0131cakl\u0131ktaki seyrek gazlarda yeterince uzun mesafeler kat edebilir, bu da \u015fok dalgas\u0131 h\u0131zland\u0131rma mekanizmas\u0131n\u0131n kozmik \u0131\u015f\u0131n par\u00e7ac\u0131klar\u0131n\u0131 etkili bir \u015fekilde h\u0131zland\u0131rmas\u0131n\u0131 m\u00fcmk\u00fcn k\u0131lar. Ancak son zamanlarda, birincil kozmik \u0131\u015f\u0131n element bollu\u011fu da\u011f\u0131l\u0131m\u0131n\u0131n atomun birinci iyonla\u015fma enerjisiyle yak\u0131ndan ili\u015fkili oldu\u011fu ke\u015ffedilmi\u015ftir: Birinci iyonla\u015fma enerjisi ne kadar d\u00fc\u015f\u00fckse, elementin birincil kozmik \u0131\u015f\u0131n bollu\u011fu o kadar y\u00fcksektir ve kozmik \u0131\u015f\u0131n kayna\u011f\u0131 ile h\u0131zlanma b\u00f6lgesinin s\u0131cakl\u0131\u011f\u0131 \u00e7ok y\u00fcksek olamaz (\u003c10^4 K), bu da s\u00fcpernovalar\u0131n...", "type": "outside"}, {"angle": -0.04656042434933738, "bbox": ["-15", "341", "654", "404"], "bg_color": ["220", "220", "220"], "fg_color": ["133", "133", "133"], "fr": "...PENDANT LE PROCESSUS DE PROPAGATION. L\u0027ORIGINE ET LA PROPAGATION DES RAYONS COSMIQUES SONT DES PRODUITS DES PROCESSUS D\u0027\u00c9VOLUTION ASTROPHYSIQUE DES HAUTES \u00c9NERGIES.", "id": "dalam proses propagasi. Asal usul dan propagasi sinar kosmik adalah produk dari proses evolusi benda langit dalam astrofisika berenergi tinggi,", "is_bold": false, "pt": "...DURANTE O PROCESSO DE PROPAGA\u00c7\u00c3O. A ORIGEM E PROPAGA\u00c7\u00c3O DOS RAIOS C\u00d3SMICOS S\u00c3O PRODUTOS DE PROCESSOS DE EVOLU\u00c7\u00c3O ASTROF\u00cdSICA DE ALTA ENERGIA,", "text": "during the propagation process. The origin and propagation of cosmic rays are products of high-energy astrophysical processes and celestial evolution,", "tr": "...yay\u0131lma s\u00fcrecinde. Kozmik \u0131\u015f\u0131nlar\u0131n k\u00f6keni ve yay\u0131l\u0131m\u0131, y\u00fcksek enerjili astrofizik ve g\u00f6k cisimlerinin evrim s\u00fcre\u00e7lerinin bir \u00fcr\u00fcn\u00fcd\u00fcr,", "type": "outside"}, {"angle": -0.05942429538902161, "bbox": ["-14", "437", "1108", "500"], "bg_color": ["222", "222", "222"], "fg_color": ["135", "135", "135"], "fr": "DURANT LEUR PROPAGATION, ILS SONT D\u00c9VI\u00c9S PAR LES CHAMPS MAGN\u00c9TIQUES, EMP\u00caCHANT DE CONNA\u00ceTRE DIRECTEMENT LEUR DISTRIBUTION SPATIALE. LEUR EXISTENCE NE PEUT \u00caTRE D\u00c9DUITE QU\u0027INDIRECTEMENT PAR LES RAYONS SECONDAIRES PRODUITS PAR L\u0027INTERACTION DES RAYONS COSMIQUES. LES RAYONS COSMIQUES, LORS DE LEUR...", "id": "selama proses propagasi dibelokkan oleh medan magnet, sehingga manusia tidak dapat secara langsung mendeteksi distribusinya di ruang angkasa, dan hanya dapat menyimpulkan keberadaannya secara tidak langsung dari sinar sekunder yang dihasilkan oleh sinar kosmik. Sinar kosmik dalam", "is_bold": false, "pt": "DURANTE A PROPAGA\u00c7\u00c3O, S\u00c3O DESVIADOS POR CAMPOS MAGN\u00c9TICOS, IMPEDINDO QUE AS PESSOAS DETECTEM DIRETAMENTE SUA DISTRIBUI\u00c7\u00c3O ESPACIAL. SUA EXIST\u00caNCIA S\u00d3 PODE SER INFERIDA INDIRETAMENTE ATRAV\u00c9S DA RADIA\u00c7\u00c3O SECUND\u00c1RIA PRODUZIDA PELOS RAIOS C\u00d3SMICOS. OS RAIOS C\u00d3SMICOS, AO INTERAGIR...", "text": "During propagation, they are deflected by magnetic fields, so people cannot directly determine their distribution in space. Their existence can only be indirectly inferred from the gamma rays produced by cosmic rays. Cosmic rays during...", "tr": "yay\u0131lma s\u0131ras\u0131nda manyetik alanlar taraf\u0131ndan sapt\u0131r\u0131l\u0131rlar, bu nedenle insanlar uzaydaki da\u011f\u0131l\u0131mlar\u0131n\u0131 do\u011frudan tespit edemezler, yaln\u0131zca kozmik \u0131\u015f\u0131nlar\u0131n \u00fcretti\u011fi ikincil radyasyon yoluyla dolayl\u0131 olarak varl\u0131klar\u0131n\u0131 \u00e7\u0131karabilirler. Kozmik \u0131\u015f\u0131nlar, [yay\u0131lma] s\u0131ras\u0131nda...", "type": "outside"}, {"angle": 0, "bbox": ["-24", "470", "1098", "695"], "bg_color": ["221", "221", "221"], "fg_color": ["133", "133", "133"], "fr": "...MOUVEMENT ET INTERACTION, \u00c9METTENT DES ONDES RADIO, DES RAYONS X, ET INTERAGISSENT CONTINUELLEMENT AVEC LA MATI\u00c8RE INTERSTELLAIRE, MODIFIANT LEUR \u00c9NERGIE ET LEUR COMPOSITION. LA COMPOSITION ET LE SPECTRE D\u0027\u00c9NERGIE DES RAYONS COSMIQUES PRIMAIRES OBSERV\u00c9S SONT D\u00c9TERMIN\u00c9S CONJOINTEMENT PAR LEUR ORIGINE PRIMORDIALE ET LEUR PROCESSUS DE PROPAGATION. POUR D\u00c9DUIRE LES CARACT\u00c9RISTIQUES DES RAYONS COSMIQUES PRIMORDIAUX \u00c0 LEUR SOURCE \u00c0 PARTIR DES OBSERVATIONS DES RAYONS COSMIQUES PRIMAIRES PR\u00c8S DE LA TERRE, IL FAUT CONSID\u00c9RER LEURS INTERACTIONS AVEC LA MATI\u00c8RE INTERSTELLAIRE PENDANT LA PROPAGATION, AINSI QUE L\u0027INFLUENCE DES CHAMPS MAGN\u00c9TIQUES TERRESTRE ET SOLAIRE. POUR D\u00c9DUIRE LA DISTRIBUTION DES PARTICULES DE RAYONS COSMIQUES DANS LA VOIE LACT\u00c9E \u00c0 PARTIR DES OBSERVATIONS RADIO, X ET GAMMA, IL FAUT AUSSI CONNA\u00ceTRE LA DISTRIBUTION DE LA MATI\u00c8RE INTERSTELLAIRE. CEPENDANT, NOTRE COMPR\u00c9HENSION DU CHAMP MAGN\u00c9TIQUE DU SYST\u00c8ME SOLAIRE ET DE CERTAINS MILIEUX INTERSTELLAIRES IMPORTANTS (COMME L\u0027HYDROG\u00c8NE MOL\u00c9CULAIRE INTERSTELLAIRE) EST ENCORE LIMIT\u00c9E. DE PLUS, AVEC LES PROGR\u00c8S DES OBSERVATIONS DES RAYONS COSMIQUES PRIMAIRES, LES LACUNES DANS LES CONNAISSANCES ACTUELLES EN PHYSIQUE NUCL\u00c9AIRE ET EN PHYSIQUE DES HAUTES \u00c9NERGIES (COMME...", "id": "gerakan dan interaksinya memancarkan gelombang radio, sinar-X, dan juga berinteraksi dengan materi antarbintang, terus mengubah energi dan komposisinya. Komposisi dan spektrum energi sinar kosmik primer yang teramati ditentukan bersama oleh asal mula dan proses propagasi. Untuk menyimpulkan kondisi sinar kosmik purba di sumbernya dari sinar kosmik primer di dekat Bumi, interaksi sinar kosmik dengan materi antarbintang selama propagasi serta medan magnet Bumi dan Tata Surya harus dipertimbangkan. Untuk menyimpulkan distribusi partikel sinar kosmik di Bima Sakti dari pengamatan radio, sinar-X, dan sinar gamma, distribusi materi antarbintang juga harus dipahami; namun, pemahaman manusia tentang medan magnet Tata Surya dan beberapa medium antarbintang penting (seperti molekul hidrogen antarbintang) baru saja dimulai. Selain itu, dengan kemajuan pengamatan sinar kosmik primer, pengetahuan fisika nuklir dan fisika energi tinggi yang ada (misalnya,", "is_bold": false, "pt": "...EMITEM ONDAS DE R\u00c1DIO, RAIOS-X, E TAMB\u00c9M INTERAGEM COM A MAT\u00c9RIA INTERESTELAR, MUDANDO CONTINUAMENTE SUA ENERGIA E COMPOSI\u00c7\u00c3O. A COMPOSI\u00c7\u00c3O E O ESPECTRO DE ENERGIA OBSERVADOS DOS RAIOS C\u00d3SMICOS PRIM\u00c1RIOS S\u00c3O DETERMINADOS TANTO PELA SUA ORIGEM PRIMITIVA QUANTO PELO PROCESSO DE PROPAGA\u00c7\u00c3O. PARA INFERIR AS CARACTER\u00cdSTICAS DOS RAIOS C\u00d3SMICOS PRIMITIVOS EM SUA FONTE A PARTIR DAS OBSERVA\u00c7\u00d5ES PR\u00d3XIMAS \u00c0 TERRA, DEVE-SE CONSIDERAR AS INTERA\u00c7\u00d5ES DOS RAIOS C\u00d3SMICOS COM A MAT\u00c9RIA INTERESTELAR DURANTE A PROPAGA\u00c7\u00c3O, BEM COMO A MODULA\u00c7\u00c3O PELOS CAMPOS MAGN\u00c9TICOS DA TERRA E DO SISTEMA SOLAR. PARA INFERIR A DISTRIBUI\u00c7\u00c3O DAS PART\u00cdCULAS DE RAIOS C\u00d3SMICOS NA VIA L\u00c1CTEA A PARTIR DE OBSERVA\u00c7\u00d5ES DE R\u00c1DIO, RAIOS-X E RAIOS GAMA, \u00c9 NECESS\u00c1RIO CONHECER A DISTRIBUI\u00c7\u00c3O DA MAT\u00c9RIA INTERESTELAR. NO ENTANTO, NOSSO CONHECIMENTO SOBRE O CAMPO MAGN\u00c9TICO DO SISTEMA SOLAR E ALGUNS MEIOS INTERESTELARES IMPORTANTES (COMO O HIDROG\u00caNIO MOLECULAR INTERESTELAR) AINDA \u00c9 INICIAL. AL\u00c9M DISSO, COM O AVAN\u00c7O DAS OBSERVA\u00c7\u00d5ES DE RAIOS C\u00d3SMICOS PRIM\u00c1RIOS, AS LIMITA\u00c7\u00d5ES DO CONHECIMENTO ATUAL DE F\u00cdSICA NUCLEAR E DE ALTAS ENERGIAS (COMO...", "text": "Radio waves and X-rays emitted during their motion and interaction, as well as continuous interactions with interstellar matter, constantly change their energy and composition.\nThe observed composition and energy spectrum of primary cosmic rays are determined by both their origin and propagation process.\nInferring the original source conditions from primary cosmic rays near Earth requires considering their interactions with interstellar matter during propagation and the effects of Earth\u0027s and the solar system\u0027s magnetic fields.\nInferring the distribution of cosmic ray particles within the Milky Way from radio, X-ray, and gamma-ray observations also requires understanding the distribution of interstellar matter.\nHowever, our understanding of the solar system\u0027s magnetic field and important interstellar media (like interstellar hydrogen molecules) recog- Furthermore, with advancements in primary cosmic ray observation, current knowledge from nuclear and high-energy physics...", "tr": "...hareket ve etkile\u015fim s\u00fcre\u00e7lerinde yay\u0131lan radyo dalgalar\u0131, X-\u0131\u015f\u0131nlar\u0131 ve gama \u0131\u015f\u0131nlar\u0131, ayr\u0131ca y\u0131ld\u0131zlararas\u0131 maddeyle etkile\u015ferek s\u00fcrekli olarak enerjilerini ve bile\u015fimlerini de\u011fi\u015ftirirler. G\u00f6zlemlenen birincil kozmik \u0131\u015f\u0131n bile\u015fimi ve enerji spektrumu, hem orijinal kaynak hem de yay\u0131lma s\u00fcreci taraf\u0131ndan ortakla\u015fa belirlenir. D\u00fcnya yak\u0131n\u0131ndaki birincil kozmik \u0131\u015f\u0131nlardan kaynak b\u00f6lgesindeki orijinal kozmik \u0131\u015f\u0131n durumunu \u00e7\u0131karmak i\u00e7in, kozmik \u0131\u015f\u0131nlar\u0131n yay\u0131lma s\u0131ras\u0131nda y\u0131ld\u0131zlararas\u0131 maddeyle etkile\u015fimini ve ayr\u0131ca D\u00fcnya ve G\u00fcne\u015f Sistemi manyetik alanlar\u0131n\u0131n etkisini dikkate almak gerekir. Radyo, X-\u0131\u015f\u0131n\u0131 ve gama \u0131\u015f\u0131n\u0131 g\u00f6zlemlerinden Samanyolu i\u00e7indeki kozmik \u0131\u015f\u0131n par\u00e7ac\u0131k da\u011f\u0131l\u0131m\u0131n\u0131 \u00e7\u0131karmak i\u00e7in, y\u0131ld\u0131zlararas\u0131 maddenin da\u011f\u0131l\u0131m\u0131n\u0131 da anlamak gerekir; ancak insanlar G\u00fcne\u015f Sistemi manyetik alan\u0131 ve baz\u0131 \u00f6nemli y\u0131ld\u0131zlararas\u0131 ortamlar (y\u0131ld\u0131zlararas\u0131 hidrojen molek\u00fclleri gibi) hakk\u0131ndaki bilgileri... Ayr\u0131ca, birincil kozmik \u0131\u015f\u0131n g\u00f6zlemlerindeki ilerlemelerle birlikte, mevcut n\u00fckleer fizik ve y\u00fcksek enerji fizi\u011fi bilgilerinin (\u00f6rne\u011fin...", "type": "outside"}, {"angle": -0.057935160583127754, "bbox": ["-2", "502", "146", "534"], "bg_color": ["222", "222", "222"], "fg_color": ["129", "129", "129"], "fr": "...LES SECTIONS EFFICACES DES R\u00c9ACTIONS NUCL\u00c9AIRES, LES DUR\u00c9ES DE VIE ET LES RAPPORTS DE BRANCHEMENT DES NUCL\u00c9IDES RADIOACTIFS \u00c0 LONGUE DUR\u00c9E DE VIE) DEVIENNENT DE PLUS EN PLUS UNE CONTRAINTE MAJEURE POUR COMPRENDRE LES RAYONS COSMIQUES PRIMORDIAUX. LES PARTICULES DE RAYONS COSMIQUES DE HAUTE \u00c9NERGIE DOIVENT PROVENIR DE DIVERS OBJETS OU PH\u00c9NOM\u00c8NES ASTROPHYSIQUES \u00c0 HAUTE \u00c9NERGIE. LE SOLEIL ET D\u0027AUTRES \u00c9TOILES, LES EXPLOSIONS DE SUPERNOVA, LES PULSARS, LES QUASARS ET LES GALAXIES ACTIVES...", "id": "dalam proses propagasi,", "is_bold": false, "pt": "DURANTE O PROCESSO DE PROPAGA\u00c7\u00c3O,", "text": "During the propagation process,", "tr": "...yay\u0131lma s\u00fcrecinde,", "type": "outside"}, {"angle": -0.037736125973651724, "bbox": ["2", "598", "115", "630"], "bg_color": ["196", "196", "196"], "fg_color": ["137", "137", "137"], "fr": "...LA MODULATION PAR LE VENT SOLAIRE,", "id": "modulasi oleh,", "is_bold": false, "pt": "A MODULA\u00c7\u00c3O DE,", "text": "...modulation,", "tr": "...mod\u00fclasyonu,", "type": "outside"}, {"angle": -0.08624295321004638, "bbox": ["-6", "662", "268", "693"], "bg_color": ["192", "192", "192"], "fg_color": ["153", "153", "153"], "fr": "...NOTRE CONNAISSANCE N\u0027EN EST QU\u0027\u00c0 SES D\u00c9BUTS.", "id": "pemahaman baru saja dimulai.", "is_bold": false, "pt": "O CONHECIMENTO AINDA EST\u00c1 APENAS COME\u00c7ANDO.", "text": "...understanding is still just beginning.", "tr": "...bilgisi hen\u00fcz ba\u015flang\u0131\u00e7 a\u015famas\u0131ndad\u0131r.", "type": "outside"}, {"angle": -1.1438191904744599e-07, "bbox": ["0", "691", "1094", "850"], "bg_color": ["221", "221", "221"], "fg_color": ["133", "133", "133"], "fr": "...LES SECTIONS EFFICACES DES R\u00c9ACTIONS NUCL\u00c9AIRES, LES DUR\u00c9ES DE VIE ET LES RAPPORTS DE BRANCHEMENT DES NUCL\u00c9IDES RADIOACTIFS \u00c0 LONGUE DUR\u00c9E DE VIE) SONT INSUFFISANTES ET LIMITENT DE PLUS EN PLUS NOTRE COMPR\u00c9HENSION. LES PARTICULES DE RAYONS COSMIQUES DE HAUTE \u00c9NERGIE DEVRAIENT PROVENIR DE DIVERS OBJETS C\u00c9LESTES \u00c0 HAUTE \u00c9NERGIE OU DE PH\u00c9NOM\u00c8NES ASTROPHYSIQUES TELS QUE LES QUASARS ET LES GALAXIES ACTIVES. PAR EXEMPLE, LES \u00c9RUPTIONS SOLAIRES PEUVENT PRODUIRE UNE PARTIE DES PARTICULES DE RAYONS COSMIQUES DANS L\u0027ESPACE DU SYST\u00c8ME SOLAIRE.", "id": "penampang reaksi nuklir, waktu paruh peluruhan dan rasio percabangan nuklida radioaktif berumur panjang) yang tidak memadai, semakin menjadi batasan. Partikel sinar kosmik berenergi tinggi seharusnya berasal dari berbagai benda langit berenergi tinggi atau quasar dan galaksi aktif berenergi tinggi, dll. Letusan jilatan api matahari di dalam Tata Surya dapat menghasilkan sebagian partikel sinar kosmik di ruang Tata Surya.", "is_bold": false, "pt": "...SE\u00c7\u00d5ES DE CHOQUE DE REA\u00c7\u00d5ES NUCLEARES, VIDAS M\u00c9DIAS DE DECAIMENTO E RAZ\u00d5ES DE RAMIFICA\u00c7\u00c3O DE NUCL\u00cdDEOS RADIOATIVOS DE LONGA DURA\u00c7\u00c3O) T\u00caM SE TORNADO CADA VEZ MAIS UM FATOR LIMITANTE. PART\u00cdCULAS DE RAIOS C\u00d3SMICOS DE ALTA ENERGIA DEVEM SE ORIGINAR DE V\u00c1RIOS OBJETOS ASTROF\u00cdSICOS DE ALTA ENERGIA, COMO QUASARES E GAL\u00c1XIAS ATIVAS. ERUP\u00c7\u00d5ES SOLARES PODEM PRODUZIR UMA PARTE DAS PART\u00cdCULAS DE RAIOS C\u00d3SMICOS NO ESPA\u00c7O DO SISTEMA SOLAR...", "text": "Due to the limitations of nuclear reaction cross-sections, decay lifetimes, and branching ratios of long-lived radionuclides, it has become increasingly important to understand the origin of high-energy cosmic ray particles, which are thought to originate from various high-energy celestial bodies or celestial high-energy processes, such as quasars and active galaxies. Solar flares can produce cosmic ray particles in the solar system space.", "tr": "...atom \u00e7ekirde\u011fi reaksiyon kesitleri, uzun \u00f6m\u00fcrl\u00fc radyoaktif n\u00fcklitlerin bozunma \u00f6m\u00fcrleri ve dallanma oranlar\u0131 gibi) eksiklikleri, kozmik \u0131\u015f\u0131nlar\u0131n anla\u015f\u0131lmas\u0131n\u0131 giderek daha fazla k\u0131s\u0131tlamaktad\u0131r. Y\u00fcksek enerjili kozmik \u0131\u015f\u0131n par\u00e7ac\u0131klar\u0131, \u00e7e\u015fitli y\u00fcksek enerjili g\u00f6k cisimleri veya kuazarlar ve aktif galaksiler gibi g\u00f6ksel y\u00fcksek enerji kaynaklar\u0131ndan kaynaklanmal\u0131d\u0131r. G\u00fcne\u015f patlamalar\u0131, G\u00fcne\u015f Sistemi uzay\u0131ndaki kozmik \u0131\u015f\u0131n par\u00e7ac\u0131klar\u0131n\u0131n bir...", "type": "outside"}, {"angle": -2.773025158830933e-06, "bbox": ["-1", "726", "435", "755"], "bg_color": ["187", "187", "187"], "fg_color": ["159", "159", "159"], "fr": "...SONT DES FACTEURS IMPORTANTS LIMITANT NOTRE COMPR\u00c9HENSION DES RAYONS COSMIQUES PRIMORDIAUX.", "id": "alasan penting mengapa orang memahami sinar kosmik purba.", "is_bold": false, "pt": "...UMA RAZ\u00c3O IMPORTANTE PARA AS PESSOAS ENTENDEREM OS RAIOS C\u00d3SMICOS PRIMITIVOS.", "text": "This is an important reason for people to understand the origin of primary cosmic rays.", "tr": "...k\u0131sm\u0131n\u0131 \u00fcretebilir, [bu da] insanlar\u0131n birincil kozmik \u0131\u015f\u0131nlar\u0131 anlamas\u0131 i\u00e7in \u00f6nemli bir nedendir.", "type": "outside"}, {"angle": 1.5198594383036834e-07, "bbox": ["-17", "759", "765", "788"], "bg_color": ["186", "186", "186"], "fg_color": ["164", "164", "164"], "fr": "...PROCESSUS. LES ACTIVIT\u00c9S \u00c0 HAUTE \u00c9NERGIE \u00c0 LA SURFACE DU SOLEIL ET D\u0027AUTRES \u00c9TOILES, LES EXPLOSIONS DE SUPERNOVA, LES PULSARS,", "id": "proses. Aktivitas berenergi tinggi di permukaan Matahari dan bintang lain, ledakan supernova, pulsar,", "is_bold": false, "pt": "PROCESSO. ATIVIDADES DE ALTA ENERGIA NA SUPERF\u00cdCIE DO SOL E DE OUTRAS ESTRELAS, EXPLOS\u00d5ES DE SUPERNOVAS, PULSARES,", "text": "High-energy activities on the surface of the Sun and other stars, supernova explosions, pulsars,", "tr": "s\u00fcre\u00e7tir. G\u00fcne\u015f ve di\u011fer y\u0131ld\u0131zlar\u0131n y\u00fczeylerindeki y\u00fcksek enerjili faaliyetler, s\u00fcpernova patlamalar\u0131, pulsarlar,", "type": "outside"}, {"angle": -0.017490311702601957, "bbox": ["-1", "790", "896", "821"], "bg_color": ["187", "187", "187"], "fg_color": ["180", "180", "180"], "fr": "...POURRAIENT \u00caTRE DES SOURCES DE RAYONS COSMIQUES. ACTUELLEMENT, ON PENSE G\u00c9N\u00c9RALEMENT QUE LA PLUPART DES PARTICULES DE RAYONS COSMIQUES PROVIENNENT DE LA VOIE LACT\u00c9E.", "id": "mungkin merupakan sumber sinar kosmik. Saat ini, secara umum diyakini bahwa sebagian besar partikel sinar kosmik berasal dari Bima Sakti.", "is_bold": false, "pt": "PODEM SER FONTES DE RAIOS C\u00d3SMICOS. ATUALMENTE, ACREDITA-SE AMPLAMENTE QUE A MAIORIA DAS PART\u00cdCULAS DE RAIOS C\u00d3SMICOS SE ORIGINA NA VIA L\u00c1CTEA.", "text": "May be the source of cosmic rays. It is now generally accepted that most cosmic ray particles originate from the Milky Way.", "tr": "kozmik \u0131\u015f\u0131n kaynaklar\u0131 olabilir. \u015eu anda, \u00e7o\u011fu insan\u0131n kozmik \u0131\u015f\u0131n par\u00e7ac\u0131klar\u0131n\u0131n \u00e7o\u011funun Samanyolu Galaksisi\u0027nden kaynakland\u0131\u011f\u0131na inand\u0131\u011f\u0131 yayg\u0131n bir g\u00f6r\u00fc\u015ft\u00fcr.", "type": "outside"}, {"angle": -0.09134839416554996, "bbox": ["-22", "821", "642", "851"], "bg_color": ["222", "222", "222"], "fg_color": ["133", "133", "133"], "fr": "CES PROCESSUS \u00c0 HAUTE \u00c9NERGIE S\u0027ACCOMPAGNENT DE L\u0027\u00c9MISSION DE PARTICULES, MAIS CE TYPE D\u0027ACTIVIT\u00c9 SOLAIRE NE PRODUIT...", "id": "proses berenergi tinggi lainnya disertai dengan emisi partikel, tetapi aktivitas matahari semacam ini hanya", "is_bold": false, "pt": "PROCESSOS DE ALTA ENERGIA S\u00c3O ACOMPANHADOS PELA EMISS\u00c3O DE PART\u00cdCULAS, MAS ESSE TIPO DE ATIVIDADE SOLAR APENAS...", "text": "Such solar activity only accounts for", "tr": "gibi y\u00fcksek enerjili s\u00fcre\u00e7lere par\u00e7ac\u0131k emisyonu e\u015flik eder, ancak bu t\u00fcr g\u00fcne\u015f aktivitesi yaln\u0131zca...", "type": "outside"}, {"angle": 0.1811129126273272, "bbox": ["-22", "852", "1078", "946"], "bg_color": ["192", "192", "192"], "fg_color": ["156", "156", "156"], "fr": "...QU\u0027UNE PETITE FRACTION, ET L\u0027\u00c9NERGIE MOYENNE DES PARTICULES SOLAIRES N\u0027EST QUE DE QUELQUES DIZAINES DE MEV. LA PLUPART DES RAYONS COSMIQUES DOIVENT PROVENIR DE L\u0027EXT\u00c9RIEUR DU SYST\u00c8ME SOLAIRE. L\u0027\u00c9MISSION DE PARTICULES PAR LES \u00c9TOILES ORDINAIRES DE LA VOIE LACT\u00c9E NE PEUT PRODUIRE QU\u0027UNE PARTIE N\u00c9GLIGEABLE DES PARTICULES DE RAYONS COSMIQUES AU SEIN DE LA GALAXIE. LES \u00c9V\u00c9NEMENTS LES PLUS VIOLENTS AU SEIN DE LA GALAXIE...", "id": "menyumbang sebagian kecil, dan energi rata-rata partikel matahari hanya beberapa puluh MeV. Sebagian besar sinar kosmik seharusnya berasal dari luar Tata Surya. Emisi partikel dari bintang biasa di Bima Sakti hanya dapat menghasilkan sebagian kecil partikel sinar kosmik di Bima Sakti; yang paling dahsyat di galaksi adalah", "is_bold": false, "pt": "...PRODUZ UMA PEQUENA FRA\u00c7\u00c3O, E A ENERGIA M\u00c9DIA DAS PART\u00cdCULAS SOLARES \u00c9 DE APENAS ALGUMAS DEZENAS DE MEV. A MAIORIA DOS RAIOS C\u00d3SMICOS DEVE VIR DE FORA DO SISTEMA SOLAR. A EMISS\u00c3O DE PART\u00cdCULAS POR ESTRELAS COMUNS DA VIA L\u00c1CTEA S\u00d3 PODE PRODUZIR UMA PARTE INSIGNIFICANTE DAS PART\u00cdCULAS DE RAIOS C\u00d3SMICOS DENTRO DA GAL\u00c1XIA. OS MAIS VIOLENTOS...", "text": "A small part, and the average energy of solar particles is only tens of mega-electron volts, so most cosmic rays should come from outside the solar system. Particle emissions from ordinary stars in the Milky Way can only produce an insignificant part of the cosmic ray particles in the Milky Way. The strongest", "tr": "...k\u00fc\u00e7\u00fck bir k\u0131sm\u0131n\u0131 olu\u015fturur ve g\u00fcne\u015f par\u00e7ac\u0131klar\u0131n\u0131n ortalama enerjisi yaln\u0131zca onlarca MeV\u0027dir; kozmik \u0131\u015f\u0131nlar\u0131n \u00e7o\u011fu G\u00fcne\u015f Sistemi d\u0131\u015f\u0131ndan gelmelidir. Samanyolu\u0027ndaki s\u0131radan y\u0131ld\u0131zlar\u0131n par\u00e7ac\u0131k emisyonu, Samanyolu i\u00e7indeki kozmik \u0131\u015f\u0131n par\u00e7ac\u0131klar\u0131n\u0131n yaln\u0131zca ihmal edilebilir bir k\u0131sm\u0131n\u0131 \u00fcretebilir; \u00e7o\u011fu [kozmik \u0131\u015f\u0131n] en \u015fiddetli...", "type": "outside"}, {"angle": -2.36584253343608e-06, "bbox": ["-9", "918", "936", "948"], "bg_color": ["185", "185", "185"], "fg_color": ["170", "170", "170"], "fr": "...LA PLUPART DES RAYONS COSMIQUES DEVRAIENT \u00caTRE PRODUITS PAR DES PROCESSUS PLUS VIOLENTS QUE L\u0027ACTIVIT\u00c9 STELLAIRE ORDINAIRE. LES EXPLOSIONS DE SUPERNOVA SONT LES PH\u00c9NOM\u00c8NES LES PLUS \u00c9NERG\u00c9TIQUES DE LA VOIE LACT\u00c9E.", "id": "sebagian sinar kosmik seharusnya dihasilkan dari proses yang lebih dahsyat daripada aktivitas bintang biasa. Ledakan supernova adalah yang paling dahsyat di Bima Sakti.", "is_bold": false, "pt": "...PROCESSOS DA GAL\u00c1XIA. A MAIORIA DOS RAIOS C\u00d3SMICOS DEVE SER PRODUZIDA POR PROCESSOS MAIS VIOLENTOS DO QUE A ATIVIDADE ESTELAR COMUM. AS EXPLOS\u00d5ES DE SUPERNOVAS S\u00c3O OS FEN\u00d4MENOS DE MAIS ALTA ENERGIA NA VIA L\u00c1CTEA.", "text": "Part of the cosmic rays should be produced by processes more intense than ordinary stellar activity. Supernova explosions are the most intense", "tr": "...kozmik \u0131\u015f\u0131nlar, s\u0131radan y\u0131ld\u0131z faaliyetlerinden daha \u015fiddetli s\u00fcre\u00e7lerde \u00fcretilmelidir. S\u00fcpernova patlamalar\u0131 Samanyolu Galaksisi\u0027ndeki...", "type": "outside"}, {"angle": -0.022665030886315662, "bbox": ["-31", "949", "1114", "1076"], "bg_color": ["221", "221", "221"], "fg_color": ["133", "133", "133"], "fr": "L\u0027\u00c9NERGIE MOYENNE \u00c9MISE PAR LES EXPLOSIONS DE SUPERNOVA DANS LA VOIE LACT\u00c9E PEUT SUFFIRE \u00c0 MAINTENIR LA DENSIT\u00c9 D\u0027\u00c9NERGIE DES RAYONS COSMIQUES GALACTIQUES. LES R\u00c9MANENTS DE SUPERNOVA, TELS QUE LA N\u00c9BULEUSE DU CRABE, \u00c9METTENT FORTEMENT UN RAYONNEMENT RADIO NON THERMIQUE HAUTEMENT POLARIS\u00c9, QUI DOIT \u00caTRE UN RAYONNEMENT SYNCHROTRON D\u0027\u00c9LECTRONS DE HAUTE \u00c9NERGIE. LA PR\u00c9SENCE D\u0027UN GRAND NOMBRE D\u0027\u00c9LECTRONS DE HAUTE \u00c9NERGIE DANS LES R\u00c9MANENTS DE SUPERNOVA SUGG\u00c8RE QU\u0027ILS SONT LA SOURCE DES \u00c9LECTRONS COSMIQUES DE HAUTE \u00c9NERGIE. ON SUPPOSE G\u00c9N\u00c9RALEMENT QUE LES EXPLOSIONS DE SUPERNOVA ET LEURS R\u00c9MANENTS DEVRAIENT \u00c9GALEMENT \u00c9METTRE DES NOYAUX ATOMIQUES DE HAUTE \u00c9NERGIE, DEVENANT AINSI LA PRINCIPALE SOURCE DE RAYONS COSMIQUES.", "id": "fenomena berenergi tinggi. Output energi rata-rata dari ledakan supernova di Bima Sakti dapat memenuhi kebutuhan untuk mempertahankan kepadatan energi sinar kosmik Bima Sakti. Sisa-sisa supernova seperti Nebula Kepiting memancarkan radiasi radio non-termal yang sangat terpolarisasi, yang seharusnya merupakan radiasi sinkrotron dari elektron berenergi tinggi. Ada banyak elektron berenergi tinggi di sisa-sisa supernova, yang seharusnya menjadi tempat asal elektron sinar kosmik berenergi tinggi. Secara umum dibayangkan bahwa ledakan supernova dan sisa-sisanya juga harus memancarkan inti atom berenergi tinggi, menjadi sumber utama sinar kosmik.", "is_bold": false, "pt": "A PRODU\u00c7\u00c3O M\u00c9DIA DE ENERGIA DAS EXPLOS\u00d5ES DE SUPERNOVAS NA VIA L\u00c1CTEA PODE SATISFAZER A NECESSIDADE DE MANTER A DENSIDADE DE ENERGIA DOS RAIOS C\u00d3SMICOS GAL\u00c1CTICOS. REMANESCENTES DE SUPERNOVAS, COMO A NEBULOSA DO CARANGUEJO, EMITEM FORTEMENTE RADIA\u00c7\u00c3O DE R\u00c1DIO N\u00c3O T\u00c9RMICA ALTAMENTE POLARIZADA, QUE DEVE SER RADIA\u00c7\u00c3O SINCROTRON DE EL\u00c9TRONS DE ALTA ENERGIA. H\u00c1 UM GRANDE N\u00daMERO DE EL\u00c9TRONS DE ALTA ENERGIA EM REMANESCENTES DE SUPERNOVAS, QUE DEVEM SER A FONTE DOS EL\u00c9TRONS DE ALTA ENERGIA DOS RAIOS C\u00d3SMICOS. \u00c9 GERALMENTE CONCEBIDO QUE AS EXPLOS\u00d5ES DE SUPERNOVAS E SEUS REMANESCENTES TAMB\u00c9M DEVEM EMITIR N\u00daCLEOS AT\u00d4MICOS DE ALTA ENERGIA, TORNANDO-SE A PRINCIPAL FONTE DE RAIOS C\u00d3SMICOS.", "text": "High-energy phenomena in the Milky Way. The average energy output of supernova explosions in the Milky Way can meet the needs of maintaining the energy density of galactic cosmic rays. Supernova remnants such as the Crab Nebula emit highly polarized non-thermal radio radiation, which should be the synchrotron radiation of high-energy electrons. There are a large number of high-energy electrons in supernova remnants, which should be the source of cosmic ray high-energy electrons. It is generally assumed that supernova explosions and their remnants should also emit high-energy atomic nuclei, becoming the main", "tr": "...y\u00fcksek enerjili olaylard\u0131r. Samanyolu\u0027ndaki s\u00fcpernova patlamalar\u0131n\u0131n ortalama enerji \u00e7\u0131kt\u0131s\u0131, galaktik kozmik \u0131\u015f\u0131n enerji yo\u011funlu\u011funu s\u00fcrd\u00fcrme ihtiyac\u0131n\u0131 kar\u015f\u0131layabilir. Yenge\u00e7 Bulutsusu gibi s\u00fcpernova kal\u0131nt\u0131lar\u0131, g\u00fc\u00e7l\u00fc bir \u015fekilde y\u00fcksek derecede polarize olmu\u015f termal olmayan radyo radyasyonu yayar; bunlar y\u00fcksek enerjili elektronlar\u0131n senkrotron radyasyonu olmal\u0131d\u0131r. S\u00fcpernova kal\u0131nt\u0131lar\u0131nda \u00e7ok say\u0131da y\u00fcksek enerjili elektron bulunur ve bunlar kozmik \u0131\u015f\u0131n y\u00fcksek enerjili elektronlar\u0131n\u0131n kaynak yeri olmal\u0131d\u0131r. \u0130nsanlar genellikle s\u00fcpernova patlamalar\u0131n\u0131n ve kal\u0131nt\u0131lar\u0131n\u0131n da y\u00fcksek enerjili atom \u00e7ekirdekleri yaymas\u0131 ve kozmik \u0131\u015f\u0131nlar\u0131n ana...", "type": "outside"}, {"angle": -0.019999267189263037, "bbox": ["2", "1014", "106", "1045"], "bg_color": ["197", "197", "197"], "fg_color": ["133", "133", "133"], "fr": "...DANS LES CHAMPS MAGN\u00c9TIQUES.", "id": "dalam medan magnet", "is_bold": false, "pt": "EM CAMPOS MAGN\u00c9TICOS.", "text": "Source of cosmic rays. The relative abundances of hydrogen and helium nuclei in cosmic rays are lower than the average abundances in the solar system or the Milky Way, indicating that cosmic ray nuclei may come from the late stages of stellar evolution. There are more heavy elements (e.g., Z\u003e60) in cosmic rays, which may be formed through the rapid neutron capture process under supernova", "tr": "manyetik alanlarda [kayna\u011f\u0131] olmas\u0131 gerekti\u011fini d\u00fc\u015f\u00fcn\u00fcr.", "type": "outside"}, {"angle": -0.02150705282426202, "bbox": ["-29", "1077", "1103", "1140"], "bg_color": ["222", "222", "222"], "fg_color": ["133", "133", "133"], "fr": "L\u0027ABONDANCE RELATIVE DES NOYAUX D\u0027HYDROG\u00c8NE ET D\u0027H\u00c9LIUM DANS LES RAYONS COSMIQUES EST INF\u00c9RIEURE \u00c0 L\u0027ABONDANCE MOYENNE DANS LE SYST\u00c8ME SOLAIRE OU LA VOIE LACT\u00c9E, CE QUI INDIQUE QUE LES NOYAUX DES RAYONS COSMIQUES POURRAIENT PROVENIR DES DERNIERS STADES DE L\u0027\u00c9VOLUTION STELLAIRE. LES RAYONS COSMIQUES CONTIENNENT UNE PROPORTION PLUS \u00c9LEV\u00c9E D\u0027\u00c9L\u00c9MENTS LOURDS (PAR EXEMPLE, Z \u003e 60), QUI POURRAIENT \u00caTRE DES PRODUITS DU PROCESSUS DE CAPTURE RAPIDE DE NEUTRONS (PROCESSUS R) DANS DES CONDITIONS DE SUPERNOVA.", "id": "sumber. Kelimpahan relatif inti hidrogen dan helium dalam sinar kosmik lebih kecil dari kelimpahan rata-rata di Tata Surya atau Bima Sakti, menunjukkan bahwa inti atom sinar kosmik mungkin berasal dari tahap akhir evolusi bintang. Ada lebih banyak unsur berat (misalnya Z\u003e60) dalam sinar kosmik, yang mungkin merupakan produk dari supernova", "is_bold": false, "pt": "A ABUND\u00c2NCIA RELATIVA DE N\u00daCLEOS DE HIDROG\u00caNIO E H\u00c9LIO NOS RAIOS C\u00d3SMICOS \u00c9 MENOR DO QUE A ABUND\u00c2NCIA M\u00c9DIA NO SISTEMA SOLAR OU NA VIA L\u00c1CTEA, INDICANDO QUE OS N\u00daCLEOS DOS RAIOS C\u00d3SMICOS PODEM VIR DOS EST\u00c1GIOS FINAIS DA EVOLU\u00c7\u00c3O ESTELAR. H\u00c1 MAIS ELEMENTOS PESADOS (POR EXEMPLO, Z\u003e60) NOS RAIOS C\u00d3SMICOS; ELES PODEM SER PRODUTOS DO PROCESSO DE CAPTURA R\u00c1PIDA DE N\u00caUTRONS (PROCESSO R) NAS CONDI\u00c7\u00d5ES DE EXPLOS\u00c3O DE SUPERNOVA.", "text": "Magnetic field.", "tr": "kayna\u011f\u0131d\u0131r. Kozmik \u0131\u015f\u0131nlardaki hidrojen ve helyum \u00e7ekirdeklerinin nispi bollu\u011fu, G\u00fcne\u015f Sistemi veya Samanyolu ortalama bollu\u011fundan daha d\u00fc\u015f\u00fckt\u00fcr, bu da kozmik \u0131\u015f\u0131n atom \u00e7ekirdeklerinin y\u0131ld\u0131z evriminin ge\u00e7 a\u015famalar\u0131ndan gelebilece\u011fini g\u00f6sterir. Kozmik \u0131\u015f\u0131nlarda a\u011f\u0131r elementler (\u00f6rne\u011fin Z\u003e60) daha fazlad\u0131r, bunlar s\u00fcpernova...", "type": "outside"}, {"angle": -0.028973607944408286, "bbox": ["-16", "1140", "410", "1171"], "bg_color": ["194", "194", "194"], "fg_color": ["164", "164", "164"], "fr": "...DANS LES CONDITIONS D\u0027UNE EXPLOSION DE SUPERNOVA.", "id": "proses penangkapan neutron cepat dalam kondisi ledakan", "is_bold": false, "pt": "PROCESSO DE CAPTURA R\u00c1PIDA DE N\u00caUTRONS SOB CONDI\u00c7\u00d5ES DE EXPLOS\u00c3O", "text": "Explosion conditions.", "tr": "...patlama ko\u015fullar\u0131 alt\u0131nda h\u0131zl\u0131 n\u00f6tron yakalama s\u00fcrecinin (r-s\u00fcreci)...", "type": "outside"}, {"angle": 1.1381651078876053e-06, "bbox": ["424", "1141", "1093", "1171"], "bg_color": ["222", "222", "222"], "fg_color": ["133", "133", "133"], "fr": "LA PLUS GRANDE ABONDANCE D\u0027ISOTOPES RICHES EN NEUTRONS DE CERTAINS \u00c9L\u00c9MENTS DANS LES RAYONS COSMIQUES...", "id": "produk dari proses r). Beberapa unsur dalam sinar kosmik memiliki lebih banyak isotop kaya neutron,", "is_bold": false, "pt": "PRODUTOS DO PROCESSO). A MAIOR ABUND\u00c2NCIA DE IS\u00d3TOPOS RICOS EM N\u00caUTRONS DE ALGUNS ELEMENTOS NOS RAIOS C\u00d3SMICOS...", "text": "product of the process). Cosmic rays have a higher abundance of neutron-rich isotopes for some elements,", "tr": "...\u00fcr\u00fcnleridir. Kozmik \u0131\u015f\u0131nlardaki baz\u0131 elementlerin n\u00f6tronca zengin izotoplar\u0131 daha...", "type": "outside"}, {"angle": -0.05108705788995849, "bbox": ["-40", "1172", "1117", "1204"], "bg_color": ["196", "196", "196"], "fg_color": ["166", "166", "166"], "fr": "...SUGG\u00c8RE \u00c9GALEMENT QUE LES RAYONS COSMIQUES POURRAIENT PROVENIR D\u0027ENVIRONNEMENTS RICHES EN NEUTRONS FORM\u00c9S LORS D\u0027EXPLOSIONS DE SUPERNOVA. CEPENDANT, IL N\u0027EXISTE \u00c0 CE JOUR AUCUNE PREUVE DIRECTE...", "id": "yang juga menunjukkan bahwa sinar kosmik mungkin berasal dari lingkungan kaya neutron yang terbentuk oleh ledakan supernova. Namun, sejauh ini tidak ada bukti langsung", "is_bold": false, "pt": "...TAMB\u00c9M INDICA QUE OS RAIOS C\u00d3SMICOS PODEM SE ORIGINAR EM AMBIENTES RICOS EM N\u00caUTRONS FORMADOS POR EXPLOS\u00d5ES DE SUPERNOVAS. NO ENTANTO, AT\u00c9 AGORA, N\u00c3O H\u00c1 EVID\u00caNCIA DIRETA...", "text": "which also indicates that cosmic rays might originate from the neutron-rich environment formed by supernova explosions. However, so far there is no direct", "tr": "...fazlad\u0131r, bu da kozmik \u0131\u015f\u0131nlar\u0131n s\u00fcpernova patlamalar\u0131n\u0131n olu\u015fturdu\u011fu n\u00f6tronca zengin ortamlardan kaynaklanabilece\u011fini g\u00f6sterir. Ancak, bug\u00fcne kadar do\u011frudan bir...", "type": "outside"}, {"angle": 0, "bbox": ["-40", "1206", "1100", "1363"], "bg_color": ["222", "222", "222"], "fg_color": ["133", "133", "133"], "fr": "...QUE LES SUPERNOVAE ET LEURS R\u00c9MANENTS \u00c9METTENT DES NOYAUX ATOMIQUES DE HAUTE \u00c9NERGIE. COMMENT L\u0027\u00c9NERGIE LIB\u00c9R\u00c9E PAR LES EXPLOSIONS DE SUPERNOVA EST CONVERTIE EN \u00c9NERGIE CIN\u00c9TIQUE DES PARTICULES, ET COMMENT DE NOMBREUSES SOURCES DISCR\u00c8TES TELLES QUE LES SUPERNOVAE PEUVENT FORMER LE SPECTRE D\u0027\u00c9NERGIE EN LOI DE PUISSANCE DES PARTICULES DE RAYONS COSMIQUES, SONT DES DIFFICULT\u00c9S POUR LES MOD\u00c8LES D\u0027ORIGINE SUPERNOVA. L\u0027ANALYSE DES R\u00c9SULTATS R\u00c9CENTS DE MESURE DE L\u0027ABONDANCE DES \u00c9L\u00c9MENTS DES RAYONS COSMIQUES PRIMAIRES MONTRE QUE LA DISTRIBUTION PRIMORDIALE DIFF\u00c8RE CONSID\u00c9RABLEMENT DES PR\u00c9DICTIONS DES MOD\u00c8LES DE PROCESSUS R. FERMI A PROPOS\u00c9 EN 1949 UN M\u00c9CANISME D\u0027ACC\u00c9L\u00c9RATION STATISTIQUE DES RAYONS COSMIQUES DANS LE MILIEU INTERSTELLAIRE.", "id": "yang menunjukkan bahwa supernova dan sisa-sisanya memancarkan inti atom berenergi tinggi. Bagaimana energi yang dilepaskan oleh ledakan supernova diubah menjadi energi kinetik partikel, dan bagaimana spektrum energi hukum pangkat partikel sinar kosmik dapat terbentuk dari banyak sumber diskrit seperti supernova, semuanya adalah masalah. Analisis hasil pengukuran terbaru kelimpahan unsur sinar kosmik primer menunjukkan bahwa distribusi purba sangat berbeda dari yang diharapkan oleh proses r. Fermi pada tahun 1949 mengusulkan mekanisme percepatan statistik sinar kosmik di medium antarbintang.", "is_bold": false, "pt": "...DE QUE SUPERNOVAS E SEUS REMANESCENTES EMITEM N\u00daCLEOS AT\u00d4MICOS DE ALTA ENERGIA. COMO A ENERGIA LIBERADA PELAS EXPLOS\u00d5ES DE SUPERNOVAS \u00c9 CONVERTIDA EM ENERGIA CIN\u00c9TICA DAS PART\u00cdCULAS, E COMO UM ESPECTRO DE ENERGIA EM LEI DE POT\u00caNCIA PARA AS PART\u00cdCULAS DE RAIOS C\u00d3SMICOS PODE SER FORMADO A PARTIR DE MUITAS FONTES DISCRETAS COMO SUPERNOVAS, S\u00c3O DIFICULDADES PARA O MODELO DE ORIGEM EM SUPERNOVAS. AN\u00c1LISES DE MEDI\u00c7\u00d5ES RECENTES DA ABUND\u00c2NCIA ELEMENTAR DOS RAIOS C\u00d3SMICOS PRIM\u00c1RIOS MOSTRAM QUE A DISTRIBUI\u00c7\u00c3O DIFERE SIGNIFICATIVAMENTE DAS PREVIS\u00d5ES DO PROCESSO R. FERMI PROP\u00d4S EM 1949 UM MECANISMO DE ACELERA\u00c7\u00c3O ESTAT\u00cdSTICA DE RAIOS C\u00d3SMICOS NO MEIO INTERESTELAR.", "text": "evidence showing that supernovae and their remnants emit high-energy atomic nuclei. How the energy released by supernova explosions converts into particle kinetic energy, and how numerous discrete sources like supernovae can form the power-law energy spectrum of cosmic ray particles, are all challenges", "tr": "...kan\u0131t yoktur ki s\u00fcpernovalar ve kal\u0131nt\u0131lar\u0131 y\u00fcksek enerjili atom \u00e7ekirdekleri yays\u0131n. S\u00fcpernova patlamalar\u0131nda sal\u0131nan enerjinin par\u00e7ac\u0131klar\u0131n kinetik enerjisine nas\u0131l d\u00f6n\u00fc\u015ft\u00fc\u011f\u00fc ve bir\u00e7ok s\u00fcpernova gibi ayr\u0131k kaynaklardan kozmik \u0131\u015f\u0131n par\u00e7ac\u0131klar\u0131n\u0131n g\u00fc\u00e7 yasas\u0131 enerji spektrumunun nas\u0131l olu\u015fabilece\u011fi, s\u00fcpernova [k\u00f6ken modeli i\u00e7in] zorluklard\u0131r. Birincil kozmik \u0131\u015f\u0131n element bolluklar\u0131n\u0131n son \u00f6l\u00e7\u00fcm sonu\u00e7lar\u0131n\u0131n analizi, orijinal ve s\u00fcre\u00e7 taraf\u0131ndan beklenen da\u011f\u0131l\u0131m aras\u0131nda b\u00fcy\u00fck bir fark oldu\u011funu g\u00f6stermektedir. Fermi, 1949\u0027da kozmik \u0131\u015f\u0131nlar\u0131n y\u0131ld\u0131zlararas\u0131 ortamda istatistiksel olarak h\u0131zland\u0131r\u0131lmas\u0131 mekanizmas\u0131n\u0131 \u00f6nermi\u015fti...", "type": "outside"}, {"angle": -0.01024955741226563, "bbox": ["-14", "1269", "359", "1299"], "bg_color": ["220", "220", "220"], "fg_color": ["132", "132", "132"], "fr": "...DIFFICULT\u00c9S RENCONTR\u00c9ES PAR LE MOD\u00c8LE D\u0027ORIGINE STELLAIRE (SUPERNOVA).", "id": "kesulitan yang dihadapi oleh model asal supernova.", "is_bold": false, "pt": "DIFICULDADES ENFRENTADAS PELO MODELO DE ORIGEM EM SUPERNOVAS.", "text": "faced by the supernova origin model.", "tr": "...y\u0131ld\u0131z k\u00f6kenli modelin kar\u015f\u0131la\u015ft\u0131\u011f\u0131 zorluklard\u0131r.", "type": "outside"}, {"angle": 6.932428092909504e-05, "bbox": ["-25", "1300", "1090", "1394"], "bg_color": ["224", "224", "224"], "fg_color": ["133", "133", "133"], "fr": "LA DISTRIBUTION DE L\u0027ABONDANCE RELATIVE DES \u00c9L\u00c9MENTS LOURDS DES RAYONS COSMIQUES EST PROCHE DE CELLE DU SYST\u00c8ME SOLAIRE, CE QUI EST INCOMPATIBLE AVEC LE MOD\u00c8LE D\u0027ORIGINE SUPERNOVA. LES PARTICULES SONT ACC\u00c9L\u00c9R\u00c9ES PAR DES COLLISIONS R\u00c9P\u00c9T\u00c9ES AVEC LES CHAMPS MAGN\u00c9TIQUES MOBILES. LE M\u00c9CANISME D\u0027ACC\u00c9L\u00c9RATION DE FERMI PEUT EXPLIQUER LE SPECTRE D\u0027\u00c9NERGIE EN LOI DE PUISSANCE DES RAYONS COSMIQUES.", "id": "Distribusi kelimpahan relatif unsur berat sinar kosmik mendekati distribusi Tata Surya, yang tidak konsisten dengan model asal supernova. ...dipercepat melalui tabrakan terus-menerus dengan medan magnet. Mekanisme percepatan Fermi dapat menjelaskan alam semesta", "is_bold": false, "pt": "A DISTRIBUI\u00c7\u00c3O DA ABUND\u00c2NCIA RELATIVA DE ELEMENTOS PESADOS NOS RAIOS C\u00d3SMICOS \u00c9 PR\u00d3XIMA \u00c0 DISTRIBUI\u00c7\u00c3O DO SISTEMA SOLAR, O QUE \u00c9 INCONSISTENTE COM O MODELO DE ORIGEM EM SUPERNOVAS. PART\u00cdCULAS S\u00c3O ACELERADAS POR COLIS\u00d5ES REPETIDAS COM CAMPOS MAGN\u00c9TICOS EM MOVIMENTO. O MECANISMO DE ACELERA\u00c7\u00c3O DE FERMI PODE EXPLICAR O ESPECTRO DE ENERGIA EM LEI DE POT\u00caNCIA DOS RAIOS C\u00d3SMICOS.", "text": "The relative abundance distribution of heavy elements in cosmic rays is close to that of the solar system, inconsistent with the supernova origin model. ...accelerated through continuous collisions with magnetic fields. The Fermi acceleration mechanism can explain the cosmic", "tr": "Kozmik \u0131\u015f\u0131n a\u011f\u0131r elementlerinin nispi bolluk da\u011f\u0131l\u0131m\u0131 G\u00fcne\u015f Sistemi da\u011f\u0131l\u0131m\u0131na yak\u0131nd\u0131r, bu da s\u00fcpernova k\u00f6ken modeliyle tutars\u0131zd\u0131r. [Par\u00e7ac\u0131klar] manyetik alanlarla s\u00fcrekli \u00e7arp\u0131\u015farak h\u0131zlan\u0131r. Fermi h\u0131zland\u0131rma mekanizmas\u0131 kozmik...", "type": "outside"}, {"angle": 8.654437266386594e-06, "bbox": ["-48", "1396", "1128", "1491"], "bg_color": ["224", "224", "224"], "fg_color": ["134", "134", "134"], "fr": "CEPENDANT, LE M\u00c9CANISME DE FERMI N\u00c9CESSITE UN PROCESSUS D\u0027INJECTION INITIAL POUR LES PARTICULES ET UNE SOURCE D\u0027\u00c9NERGIE SUFFISANTE POUR LE MOUVEMENT DES CHAMPS MAGN\u00c9TIQUES DANS LE MILIEU INTERSTELLAIRE. DE PLUS, LE M\u00c9CANISME DE FERMI EST MOINS EFFICACE POUR ACC\u00c9L\u00c9RER LES NOYAUX LOURDS, CE QUI REND DIFFICILE L\u0027EXPLICATION DES ABONDANCES OBSERV\u00c9ES DANS LES RAYONS COSMIQUES. DES ONDES DE CHOC INTENSES EXISTENT DANS LES R\u00c9MANENTS DE SUPERNOVA PENDANT AU MOINS 10^4 ANS. L\u0027ANALYSE TH\u00c9ORIQUE...", "id": "spektrum energi hukum pangkat sinar. Namun, mekanisme Fermi memerlukan proses percepatan awal lain untuk partikel, dan memerlukan pasokan energi yang cukup untuk medan magnet di medium antarbintang; pada saat yang sama, mekanisme Fermi tidak mendukung percepatan inti atom berat, sehingga sulit untuk menjelaskan kelimpahan sinar kosmik yang teramati. Sisa-sisa supernova memiliki gelombang kejut yang kuat setidaknya selama 10^4 tahun. Teori", "is_bold": false, "pt": "NO ENTANTO, O MECANISMO DE FERMI REQUER UM PROCESSO DE ACELERA\u00c7\u00c3O INICIAL PARA AS PART\u00cdCULAS E UM FORNECIMENTO SUFICIENTE DE ENERGIA PARA O MOVIMENTO DOS CAMPOS MAGN\u00c9TICOS NO MEIO INTERESTELAR. AL\u00c9M DISSO, O MECANISMO DE FERMI N\u00c3O \u00c9 FAVOR\u00c1VEL \u00c0 ACELERA\u00c7\u00c3O DE N\u00daCLEOS AT\u00d4MICOS PESADOS, DIFICULTANDO A EXPLICA\u00c7\u00c3O DA ABUND\u00c2NCIA OBSERVADA NOS RAIOS C\u00d3SMICOS. OBSERVA\u00c7\u00d5ES DE RAIOS-X RECENTES DESCOBRIRAM QUE ONDAS DE CHOQUE FORTES EXISTEM EM REMANESCENTES DE SUPERNOVAS POR PELO MENOS 10^4 ANOS. AN\u00c1LISES TE\u00d3RICAS...", "text": "ray power-law energy spectrum. However, the Fermi mechanism requires an initial acceleration process for the particles and sufficient energy supply. Simultaneously, the Fermi mechanism is not efficient at accelerating heavy atomic nuclei, making it difficult to explain the observed cosmic ray abundance", "tr": "...\u0131\u015f\u0131nlar\u0131n\u0131n g\u00fc\u00e7 yasas\u0131 enerji spektrumunu a\u00e7\u0131klayabilir. Ancak, Fermi mekanizmas\u0131 par\u00e7ac\u0131klar\u0131n ba\u015fka bir ba\u015flang\u0131\u00e7 h\u0131zland\u0131rma s\u00fcrecine sahip olmas\u0131n\u0131 ve y\u0131ld\u0131zlararas\u0131 [ortamdaki] manyetik alanlar\u0131n hareketine yeterli enerji sa\u011flanmas\u0131n\u0131 gerektirir; ayn\u0131 zamanda Fermi mekanizmas\u0131 a\u011f\u0131r atom \u00e7ekirdeklerini h\u0131zland\u0131rmak i\u00e7in elveri\u015fsizdir ve g\u00f6zlemlenen kozmik \u0131\u015f\u0131n bollu\u011funu a\u00e7\u0131klamakta zorlan\u0131r. S\u00fcpernova kal\u0131nt\u0131lar\u0131nda en az 10^4 y\u0131l boyunca g\u00fc\u00e7l\u00fc \u015fok dalgalar\u0131 bulunur. Teorik...", "type": "outside"}, {"angle": -0.004304427981480785, "bbox": ["-5", "1429", "295", "1461"], "bg_color": ["193", "193", "193"], "fg_color": ["163", "163", "163"], "fr": "...MOUVEMENT DES CHAMPS MAGN\u00c9TIQUES DANS LE MILIEU INTERSTELLAIRE ;", "id": "pergerakan medan magnet di medium antarbintang;", "is_bold": false, "pt": "MOVIMENTO DE CAMPOS MAGN\u00c9TICOS NO MEIO INTERESTELAR;", "text": "motion of magnetic fields in the interstellar medium;", "tr": "...y\u0131ld\u0131zlararas\u0131 ortamdaki manyetik alanlar\u0131n hareketi;", "type": "outside"}, {"angle": -3.5675039100624417e-06, "bbox": ["-14", "1462", "419", "1492"], "bg_color": ["225", "225", "225"], "fg_color": ["135", "135", "135"], "fr": "...DISTRIBUTION D\u0027ABONDANCE. DES OBSERVATIONS R\u00c9CENTES EN RAYONS X ONT R\u00c9V\u00c9L\u00c9 QUE...", "id": "distribusi kelimpahan. Pengamatan sinar-X baru-baru ini menemukan,", "is_bold": false, "pt": "DISTRIBUI\u00c7\u00c3O DA ABUND\u00c2NCIA. OBSERVA\u00c7\u00d5ES RECENTES DE RAIOS-X DESCOBRIRAM,", "text": "distribution. Recent X-ray observations have found that,", "tr": "...bolluk da\u011f\u0131l\u0131m\u0131n\u0131. Son X-\u0131\u015f\u0131n\u0131 g\u00f6zlemleri \u015funu bulmu\u015ftur:", "type": "outside"}, {"angle": 0, "bbox": ["-32", "1494", "1047", "1523"], "bg_color": ["189", "189", "189"], "fg_color": ["160", "160", "160"], "fr": "...MONTRE QUE LES ONDES DE CHOC DANS LE MILIEU INTERSTELLAIRE PEUVENT ACC\u00c9L\u00c9RER EFFICACEMENT LES PARTICULES DES RAYONS COSMIQUES ET PRODUIRE UN SPECTRE D\u0027\u00c9NERGIE EN LOI DE PUISSANCE.", "id": "analisis menunjukkan bahwa gelombang kejut di medium antarbintang dapat secara efektif mempercepat partikel sinar kosmik dan dapat menghasilkan spektrum energi hukum pangkat.", "is_bold": false, "pt": "...MOSTRAM QUE AS ONDAS DE CHOQUE NO MEIO INTERESTELAR PODEM ACELERAR EFICAZMENTE AS PART\u00cdCULAS DE RAIOS C\u00d3SMICOS E PRODUZIR UM ESPECTRO DE ENERGIA EM LEI DE POT\u00caNCIA.", "text": "analysis indicates that shock waves in the interstellar medium can effectively accelerate cosmic ray particles and can also produce a power-law energy spectrum.", "tr": "analizler, y\u0131ld\u0131zlararas\u0131 ortamdaki \u015fok dalgalar\u0131n\u0131n kozmik \u0131\u015f\u0131n par\u00e7ac\u0131klar\u0131n\u0131 etkili bir \u015fekilde h\u0131zland\u0131rabildi\u011fini ve bir g\u00fc\u00e7 yasas\u0131 enerji spektrumu \u00fcretebildi\u011fini g\u00f6stermektedir.", "type": "outside"}, {"angle": -8.932979369546956e-06, "bbox": ["-2", "1621", "331", "1648"], "bg_color": ["210", "210", "210"], "fg_color": ["143", "143", "143"], "fr": "...PLUS LE RAPPORT \u00c0 L\u0027ABONDANCE SOLAIRE EST \u00c9LEV\u00c9. DONC,", "id": "semakin besar rasio kelimpahan terhadap Matahari. Jadi,", "is_bold": false, "pt": "QUANTO MAIOR A RAZ\u00c3O EM RELA\u00c7\u00c3O \u00c0 ABUND\u00c2NCIA SOLAR. PORTANTO,", "text": "the ratio to solar abundance is larger. Therefore,", "tr": "...G\u00fcne\u015f bollu\u011funa oran\u0131 o kadar b\u00fcy\u00fckt\u00fcr. Bu nedenle,", "type": "outside"}], "width": 1080}, {"height": 1200, "img_url": "snowmtl.ru/latest/the-original/205/12.webp", "translations": [{"angle": -0.06705641751679536, "bbox": ["174", "195", "759", "225"], "bg_color": ["203", "203", "203"], "fg_color": ["130", "130", "130"], "fr": "LORSQUE J\u0027ATTEINS LA TERRE, L\u0027ATMOSPH\u00c8RE BLOQUE UNE GRANDE PARTIE...", "id": "Ketika saya mencapai Bumi, akan ada lapisan atmosfer yang menghalangi sebagian...", "is_bold": false, "pt": "QUANDO OS RAIOS C\u00d3SMICOS ATINGEM A TERRA, A ATMOSFERA BLOQUEIA UMA PARTE DELES.", "text": "When they reach Earth, the atmosphere blocks a portion.", "tr": "D\u00fcnya\u0027ya ula\u015ft\u0131\u011f\u0131nda, atmosferin bir k\u0131sm\u0131 [taraf\u0131ndan emilir]...", "type": "outside"}, {"angle": 8.337471513186756e-08, "bbox": ["76", "226", "831", "253"], "bg_color": ["205", "205", "205"], "fg_color": ["135", "135", "135"], "fr": "...L\u0027INTENSIT\u00c9 DU FLUX DE RAYONS EST ENCORE CONSID\u00c9RABLE ET POURRAIT AVOIR UN CERTAIN IMPACT SUR LE TRAFIC A\u00c9RIEN.", "id": "intensitas aliran sinar masih sangat besar, dan sangat mungkin berdampak pada lalu lintas udara sampai batas tertentu.", "is_bold": false, "pt": "A INTENSIDADE DO FLUXO DE RAIOS AINDA \u00c9 GRANDE E PODE TER UM CERTO GRAU DE IMPACTO NO TR\u00c1FEGO A\u00c9REO.", "text": "the intensity of the ray flux is still significant, potentially affecting air traffic to some extent.", "tr": "...\u0131\u015f\u0131n ak\u0131s\u0131n\u0131n yo\u011funlu\u011fu hala \u00e7ok y\u00fcksektir ve hava trafi\u011fi \u00fczerinde belirli bir derecede [etkiye] sahip olmas\u0131 muhtemeldir.", "type": "outside"}, {"angle": -0.02431756446398481, "bbox": ["-41", "255", "1084", "521"], "bg_color": ["223", "223", "223"], "fg_color": ["134", "134", "134"], "fr": "PAR EXEMPLE, LES SYST\u00c8MES DE CONTR\u00d4LE ET DE NAVIGATION UTILIS\u00c9S DANS LES AVIONS MODERNES CONTIENNENT DES COMPOSANTS MICRO\u00c9LECTRONIQUES TR\u00c8S SENSIBLES. S\u0027ILS SONT FRAPP\u00c9S PAR DES PARTICULES CHARG\u00c9ES \u00c0 HAUTE ALTITUDE, ILS POURRAIENT TOMBER EN PANNE, CAUSANT DES PROBL\u00c8MES ET DES MENACES CONSID\u00c9RABLES POUR LE VOL. CERTAINS SCIENTIFIQUES PENSENT \u00c9GALEMENT QUE LE R\u00c9CHAUFFEMENT CLIMATIQUE, UNE PR\u00c9OCCUPATION INTERNATIONALE DE LONGUE DATE, POURRAIT \u00caTRE DIRECTEMENT LI\u00c9 AUX RAYONS COSMIQUES. SELON CE POINT DE VUE, L\u0027EFFET DE SERRE NE SERAIT PAS LE SEUL COUPABLE DU R\u00c9CHAUFFEMENT CLIMATIQUE ; LES RAYONS COSMIQUES POURRAIENT CONTRIBUER AU R\u00c9CHAUFFEMENT DE LA TERRE EN MODIFIANT LA FORMATION DES NUAGES DANS LA BASSE ATMOSPH\u00c8RE. LES RECHERCHES DE CES SCIENTIFIQUES SUGG\u00c8RENT QUE LES VARIATIONS DU NIVEAU DES RAYONS COSMIQUES POURRAIENT \u00caTRE LA CL\u00c9 POUR EXPLIQUER CE PROBL\u00c8ME COMPLEXE. ILS SOULIGNENT QUE LES PARTICULES DE HAUTE \u00c9NERGIE PROVENANT DE L\u0027ESPACE EXTRA-ATMOSPH\u00c9RIQUE \u00c9JECTENT DES \u00c9LECTRONS DES ATOMES, FORMANT DES IONS CHARG\u00c9S QUI PEUVENT PROVOQUER LA CONDENSATION DE GOUTTELETTES D\u0027EAU, AUGMENTANT AINSI LA CROISSANCE DES NUAGES. AUTREMENT DIT, LORSQUE LES RAYONS COSMIQUES SONT MOINS NOMBREUX, MOINS DE NUAGES SE FORMENT, PERMETTANT AINSI...", "id": "Menurut para ahli, sistem kontrol dan navigasi yang digunakan pada pesawat modern memiliki mikroelektronika yang cukup sensitif. Begitu diserang oleh partikel bermuatan di ketinggian, sistem tersebut dapat gagal, menimbulkan masalah dan ancaman besar bagi penerbangan. Beberapa ilmuwan juga percaya bahwa masalah pemanasan global, yang telah lama menjadi perhatian masyarakat internasional, mungkin juga terkait langsung dengan sinar kosmik. Pandangan ini menyatakan bahwa efek rumah kaca mungkin bukan satu-satunya penyebab pemanasan global; sinar kosmik dapat berkontribusi terhadap pemanasan Bumi dengan mengubah cara pembentukan awan di atmosfer bagian bawah. Penelitian para ilmuwan ini menunjukkan bahwa perubahan tingkat sinar kosmik mungkin menjadi kunci untuk menjelaskan masalah yang membingungkan ini. Mereka menunjukkan bahwa karena partikel berenergi tinggi dari luar angkasa menghantam elektron keluar dari atom, ion bermuatan yang terbentuk dapat menyebabkan kondensasi tetesan air, sehingga meningkatkan pertumbuhan awan. Artinya, ketika sinar kosmik lebih sedikit, lebih sedikit awan yang terbentuk, sehingga", "is_bold": false, "pt": "POR EXEMPLO, OS SISTEMAS DE CONTROLE E NAVEGA\u00c7\u00c3O USADOS EM AERONAVES MODERNAS POSSUEM MICROELETR\u00d4NICA BASTANTE SENS\u00cdVEL. UMA VEZ ATACADOS POR PART\u00cdCULAS CARREGADAS EM ALTAS ALTITUDES, ELES PODEM FALHAR, TRAZENDO PROBLEMAS E AMEA\u00c7AS CONSIDER\u00c1VEIS AO VOO DA AERONAVE. ALGUNS CIENTISTAS TAMB\u00c9M ACREDITAM QUE O PROBLEMA DO AQUECIMENTO GLOBAL, H\u00c1 MUITO TEMPO UMA PREOCUPA\u00c7\u00c3O DA COMUNIDADE INTERNACIONAL, PODE ESTAR DIRETAMENTE RELACIONADO AOS RAIOS C\u00d3SMICOS. ESSA VIS\u00c3O SUSTENTA QUE O EFEITO ESTUFA PODE N\u00c3O SER O \u00daNICO CULPADO PELO AQUECIMENTO GLOBAL; OS RAIOS C\u00d3SMICOS PODEM CONTRIBUIR PARA O AQUECIMENTO DA TERRA, ALTERANDO A FORMA COMO AS NUVENS SE FORMAM NA BAIXA ATMOSFERA. PESQUISAS DESSES CIENTISTAS SUGEREM QUE AS VARIA\u00c7\u00d5ES NO N\u00cdVEL DE RAIOS C\u00d3SMICOS PODEM SER A CHAVE PARA EXPLICAR ESSE PROBLEMA COMPLEXO. ELES APONTAM QUE, COMO PART\u00cdCULAS DE ALTA ENERGIA DO ESPA\u00c7O SIDERAL EJETAM EL\u00c9TRONS DOS \u00c1TOMOS, OS \u00cdONS CARREGADOS RESULTANTES PODEM CAUSAR A CONDENSA\u00c7\u00c3O DE GOT\u00cdCULAS DE \u00c1GUA, AUMENTANDO ASSIM O CRESCIMENTO DAS NUVENS. OU SEJA, QUANDO H\u00c1 MENOS RAIOS C\u00d3SMICOS, MENOS NUVENS S\u00c3O PRODUZIDAS, E ASSIM,", "text": "According to reports, the control and navigation systems used in modern aircraft contain highly sensitive microelectronics. If attacked by charged particles at high altitudes, they could malfunction, causing significant trouble and threats to flight safety. Some scientists also believe that the long-standing global concern of global warming might be directly related to cosmic rays. This view suggests that the greenhouse effect may not be the sole culprit for global warming; cosmic rays might contribute by altering cloud formation in the lower atmosphere. Research by these scientists suggests that variations in cosmic ray levels could be key to explaining this complex issue. They point out that high-energy particles from outer space knock electrons out of atoms, forming charged ions that can trigger water droplet condensation, thus increasing cloud growth. In other words, fewer cosmic rays mean fewer clouds,", "tr": "\u00d6rne\u011fin, modern u\u00e7aklarda kullan\u0131lan kontrol sistemleri ve navigasyon sistemleri olduk\u00e7a hassas mikroelektronik bile\u015fenlere sahiptir. Y\u00fcksek irtifada y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131n sald\u0131r\u0131s\u0131na u\u011frad\u0131klar\u0131nda ar\u0131zalanabilirler, bu da u\u00e7a\u011f\u0131n u\u00e7u\u015fu i\u00e7in \u00f6nemli sorunlar ve tehditler olu\u015fturur. Baz\u0131 bilim adamlar\u0131 ayr\u0131ca, uzun s\u00fcredir uluslararas\u0131 toplumun dikkatini \u00e7eken k\u00fcresel \u0131s\u0131nma sorununun da kozmik \u0131\u015f\u0131nlarla do\u011frudan ili\u015fkili olabilece\u011fine inanmaktad\u0131r. Bu g\u00f6r\u00fc\u015fe g\u00f6re, sera etkisi k\u00fcresel \u0131s\u0131nman\u0131n tek su\u00e7lusu olmayabilir; kozmik \u0131\u015f\u0131nlar, alt atmosferdeki bulut olu\u015fum \u015feklini de\u011fi\u015ftirerek D\u00fcnya\u0027n\u0131n \u0131s\u0131nmas\u0131na neden olabilir. Bu bilim adamlar\u0131n\u0131n ara\u015ft\u0131rmalar\u0131, kozmik \u0131\u015f\u0131n seviyelerindeki de\u011fi\u015fikliklerin bu karma\u015f\u0131k sorunu a\u00e7\u0131klamada anahtar olabilece\u011fini \u00f6ne s\u00fcr\u00fcyor. D\u0131\u015f uzaydan gelen y\u00fcksek enerjili par\u00e7ac\u0131klar\u0131n atomlardaki elektronlar\u0131 d\u0131\u015far\u0131 atarak y\u00fckl\u00fc iyonlar olu\u015fturdu\u011funu ve bu iyonlar\u0131n su damlac\u0131klar\u0131n\u0131n yo\u011funla\u015fmas\u0131na neden olarak bulut b\u00fcy\u00fcmesini art\u0131rabilece\u011fini belirtiyorlar. Yani, kozmik \u0131\u015f\u0131nlar daha az oldu\u011funda, daha az bulut olu\u015fur, b\u00f6ylece...", "type": "outside"}, {"angle": -6.275756106788322e-06, "bbox": ["93", "492", "1048", "520"], "bg_color": ["219", "219", "219"], "fg_color": ["136", "136", "136"], "fr": "...AU SOLEIL DE CHAUFFER DIRECTEMENT LA SURFACE DE LA TERRE. LES DONN\u00c9ES D\u0027OBSERVATION DE L\u0027ACTIVIT\u00c9 SOLAIRE ET DE SON INTENSIT\u00c9 DE RAYONNEMENT AU COURS DES 20 DERNI\u00c8RES ANN\u00c9ES...", "id": "Matahari dapat langsung memanaskan permukaan Bumi. Data pengamatan aktivitas matahari dan intensitas radioaktifnya selama 20 tahun terakhir", "is_bold": false, "pt": "O SOL PODE AQUECER DIRETAMENTE A SUPERF\u00cdCIE DA TERRA. DADOS DE OBSERVA\u00c7\u00c3O DA ATIVIDADE SOLAR E SUA INTENSIDADE DE RADIA\u00c7\u00c3O NOS \u00daLTIMOS 20 ANOS...", "text": "allowing the sun to directly heat the Earth\u0027s surface. Observational data on solar activity and its radiation intensity over the past 20 years", "tr": "...G\u00fcne\u015f do\u011frudan D\u00fcnya y\u00fczeyini \u0131s\u0131tabilir. Son 20 y\u0131ldaki g\u00fcne\u015f aktivitesi ve radyasyon yo\u011funlu\u011funa ili\u015fkin g\u00f6zlemsel veriler...", "type": "outside"}, {"angle": 0.00032781333908360466, "bbox": ["-12", "521", "1089", "616"], "bg_color": ["223", "223", "223"], "fg_color": ["134", "134", "134"], "fr": "...SOUTIENNENT CETTE NOUVELLE PERSPECTIVE : LORSQUE L\u0027ACTIVIT\u00c9 SOLAIRE DEVIENT PLUS INTENSE, LA COUVERTURE NUAGEUSE \u00c0 BASSE ALTITUDE DIMINUE. EN EFFET, LES PARTICULES CHARG\u00c9ES DE FAIBLE \u00c9NERGIE \u00c9MISES PAR LE SOLEIL (C\u0027EST-\u00c0-DIRE LE VENT SOLAIRE) PEUVENT D\u00c9VIER LES RAYONS COSMIQUES. AVEC L\u0027INTENSIFICATION DE L\u0027ACTIVIT\u00c9 SOLAIRE, LE VENT SOLAIRE SE RENFORCE \u00c9GALEMENT.", "id": "mendukung pandangan baru ini, yaitu ketika aktivitas matahari menjadi lebih intens, tutupan awan di ketinggian rendah berkurang. Ini karena partikel bermuatan berenergi rendah yang dipancarkan oleh Matahari (yaitu angin matahari) dapat membelokkan sinar kosmik. Seiring dengan meningkatnya aktivitas matahari, angin matahari juga", "is_bold": false, "pt": "...APOIAM ESSA NOVA VIS\u00c3O: QUANDO A ATIVIDADE SOLAR SE TORNA MAIS INTENSA, A COBERTURA DE NUVENS DE BAIXA ALTITUDE DIMINUI. ISSO OCORRE PORQUE AS PART\u00cdCULAS CARREGADAS DE BAIXA ENERGIA EMITIDAS PELO SOL (OU SEJA, O VENTO SOLAR) PODEM DESVIAR OS RAIOS C\u00d3SMICOS. COM O AUMENTO DA ATIVIDADE SOLAR, O VENTO SOLAR TAMB\u00c9M SE INTENSIFICA,", "text": "supports this new viewpoint: when solar activity intensifies, low-altitude cloud cover decreases. This is because low-energy charged particles emitted by the sun (i.e., solar wind) can deflect cosmic rays. As solar activity increases, the solar wind", "tr": "...bu yeni g\u00f6r\u00fc\u015f\u00fc desteklemektedir; yani, g\u00fcne\u015f aktivitesi daha \u015fiddetli hale geldi\u011finde, al\u00e7ak seviye bulut \u00f6rt\u00fcs\u00fc azal\u0131r. Bunun nedeni, G\u00fcne\u015f\u0027ten yay\u0131lan d\u00fc\u015f\u00fck enerjili y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131n (yani g\u00fcne\u015f r\u00fczgar\u0131) kozmik \u0131\u015f\u0131nlar\u0131 sapt\u0131rabilmesi ve g\u00fcne\u015f aktivitesi yo\u011funla\u015ft\u0131k\u00e7a g\u00fcne\u015f r\u00fczgar\u0131n\u0131n da...", "type": "outside"}, {"angle": -0.07081103098252584, "bbox": ["-10", "581", "1102", "817"], "bg_color": ["222", "222", "222"], "fg_color": ["133", "133", "133"], "fr": "...R\u00c9DUISANT AINSI LA QUANTIT\u00c9 DE RAYONS COSMIQUES ATTEIGNANT LA TERRE, ET DONC LA FORMATION DE NUAGES. DE PLUS, DANS LA HAUTE ATMOSPH\u00c8RE, SI LA CONCENTRATION DE PARTICULES CHARG\u00c9ES PRODUITES PAR LES RAYONS COSMIQUES EST \u00c9LEV\u00c9E, CES IONS CHARG\u00c9S PEUVENT ENTRER EN COLLISION ET SE RECOMBINER. CEPENDANT, \u00c0 BASSE ALTITUDE, LES IONS CHARG\u00c9S PERSISTENT PLUS LONGTEMPS, SUFFISAMMENT POUR PROVOQUER LA FORMATION DE NOUVEAUX NUAGES. EN OUTRE, PLUSIEURS SCIENTIFIQUES AM\u00c9RICAINS ESTIMENT QUE LES RAYONS COSMIQUES POURRAIENT \u00caTRE LI\u00c9S \u00c0 L\u0027EXTINCTION ET \u00c0 L\u0027APPARITION D\u0027ESP\u00c8CES BIOLOGIQUES. ILS PENSENT QU\u0027UNE AUGMENTATION SOUDAINE DES RAYONS COSMIQUES \u00c0 UN CERTAIN STADE POURRAIT D\u00c9TRUIRE LA COUCHE D\u0027OZONE DE LA TERRE ET AUGMENTER LA RADIOACTIVIT\u00c9 DE L\u0027ENVIRONNEMENT TERRESTRE, ENTRA\u00ceNANT DES MUTATIONS D\u0027ESP\u00c8CES, VOIRE LEUR EXTINCTION. D\u0027UN AUTRE C\u00d4T\u00c9, CES RAYONS POURRAIENT \u00c9GALEMENT INDUIRE DES MUTATIONS CHEZ DE NOUVELLES ESP\u00c8CES, DONNANT NAISSANCE \u00c0 UNE TOUTE NOUVELLE G\u00c9N\u00c9RATION. CETTE TH\u00c9ORIE SUGG\u00c8RE \u00c9GALEMENT QUE CERTAINS ORGANISMES VIVANT DANS DES GROTTES, AU FOND DES MERS OU SOUS LA SURFACE TERRESTRE N\u0027ONT PAS DISPARU PR\u00c9CIS\u00c9MENT PARCE QU\u0027ILS POUVAIENT \u00c9CHAPPER \u00c0 LA PLUPART DES RADIATIONS. DE CE POINT DE VUE, LES RAYONS COSMIQUES SONT BIEN...", "id": "menguat, sehingga lebih sedikit sinar kosmik yang mencapai Bumi, dan akibatnya lebih sedikit awan yang terbentuk. Selain itu, di ruang angkasa bagian atas, jika konsentrasi partikel bermuatan yang dihasilkan oleh sinar kosmik sangat tinggi, ion-ion bermuatan ini dapat saling bertabrakan dan bergabung kembali. Tetapi ion bermuatan di ketinggian rendah bertahan untuk waktu yang relatif lebih lama, sehingga cukup untuk menyebabkan pembentukan awan baru. Beberapa ilmuwan Amerika juga percaya bahwa sinar kosmik sangat mungkin terkait dengan kepunahan dan kemunculan spesies biologis. Mereka percaya bahwa peningkatan tiba-tiba sinar kosmik pada tahap tertentu sangat mungkin merusak lapisan ozon Bumi dan meningkatkan radioaktivitas lingkungan Bumi, yang menyebabkan mutasi atau bahkan kepunahan spesies. Di sisi lain, sinar-sinar ini juga dapat mendorong mutasi pada spesies baru, sehingga menghasilkan generasi yang sama sekali baru. Teori ini juga menunjukkan bahwa beberapa organisme yang hidup di gua, dasar laut, atau di bawah permukaan tanah tidak punah justru karena mereka dapat menghindari sebagian besar radiasi. Dari sudut pandang ini, sinar kosmik memang benar-benar", "is_bold": false, "pt": "FAZENDO COM QUE MENOS RAIOS C\u00d3SMICOS ATINJAM A TERRA, RESULTANDO EM MENOS NUVENS. AL\u00c9M DISSO, NA ALTA ATMOSFERA, SE A CONCENTRA\u00c7\u00c3O DE PART\u00cdCULAS CARREGADAS GERADAS PELOS RAIOS C\u00d3SMICOS FOR MUITO ALTA, ESSES \u00cdONS CARREGADOS PODEM COLIDIR E SE RECOMBINAR. NO ENTANTO, \u00cdONS CARREGADOS EM BAIXAS ALTITUDES PERSISTEM POR UM TEMPO RELATIVAMENTE MAIS LONGO, SENDO SUFICIENTES PARA CAUSAR A FORMA\u00c7\u00c3O DE NOVAS NUVENS. ALGUNS CIENTISTAS AMERICANOS TAMB\u00c9M ACREDITAM QUE OS RAIOS C\u00d3SMICOS PODEM ESTAR RELACIONADOS \u00c0 EXTIN\u00c7\u00c3O E AO SURGIMENTO DE ESP\u00c9CIES BIOL\u00d3GICAS. ELES TEORIZAM QUE UM AUMENTO S\u00daBITO NOS RAIOS C\u00d3SMICOS EM UM DETERMINADO EST\u00c1GIO PODERIA DESTRUIR A CAMADA DE OZ\u00d4NIO DA TERRA E AUMENTAR A RADIOATIVIDADE AMBIENTAL, LEVANDO \u00c0 MUTA\u00c7\u00c3O E AT\u00c9 \u00c0 EXTIN\u00c7\u00c3O DE ESP\u00c9CIES. POR OUTRO LADO, ESSES RAIOS TAMB\u00c9M PODERIAM INDUZIR MUTA\u00c7\u00d5ES EM NOVAS ESP\u00c9CIES, GERANDO ASSIM UMA GERA\u00c7\u00c3O COMPLETAMENTE NOVA. ESTA TEORIA TAMB\u00c9M APONTA QUE CERTOS ORGANISMOS QUE VIVEM EM CAVERNAS, NO FUNDO DO MAR OU ABAIXO DA SUPERF\u00cdCIE N\u00c3O FORAM EXTINTOS PRECISAMENTE PORQUE CONSEGUIRAM ESCAPAR DA MAIOR PARTE DA RADIA\u00c7\u00c3O. DESTE PONTO DE VISTA, OS RAIOS C\u00d3SMICOS S\u00c3O REALMENTE...", "text": "is also enhanced, causing fewer cosmic rays to reach Earth, thus forming fewer clouds. Additionally, in the upper atmosphere, if the concentration of charged particles produced by cosmic rays is high, these charged ions might collide and recombine. However, charged ions at lower altitudes persist for a relatively longer time, thus being sufficient to cause new cloud formation. Furthermore, several American scientists believe that cosmic rays are highly likely related to the extinction and emergence of biological species. They theorize that a sudden increase in cosmic rays during a certain period could potentially damage the Earth\u0027s ozone layer and increase environmental radioactivity, leading to species mutation or even extinction. On the other hand, these rays might also induce mutations in new species, thereby creating a completely new generation. This theory also points out that some organisms living in caves, underwater, or below the surface survived precisely because they could escape most of the radiation. From this perspective, cosmic rays truly are", "tr": "...g\u00fc\u00e7lenmesi, b\u00f6ylece D\u00fcnya\u0027ya ula\u015fan kozmik \u0131\u015f\u0131nlar\u0131n azalmas\u0131 ve dolay\u0131s\u0131yla daha az bulut olu\u015fmas\u0131d\u0131r. Ayr\u0131ca, y\u00fcksek atmosferde, e\u011fer kozmik \u0131\u015f\u0131nlar\u0131n \u00fcretti\u011fi y\u00fckl\u00fc par\u00e7ac\u0131k konsantrasyonu \u00e7ok y\u00fcksekse, bu y\u00fckl\u00fc iyonlar birbirleriyle \u00e7arp\u0131\u015fabilir ve yeniden birle\u015febilir. Ancak al\u00e7ak atmosferdeki y\u00fckl\u00fc iyonlar nispeten daha uzun s\u00fcre kal\u0131r, bu nedenle yeni bulut olu\u015fumuna neden olmak i\u00e7in yeterlidirler. Bu birka\u00e7 Amerikal\u0131 bilim adam\u0131 ayr\u0131ca, kozmik \u0131\u015f\u0131nlar\u0131n biyolojik t\u00fcrlerin yok olmas\u0131 ve ortaya \u00e7\u0131kmas\u0131yla da ilgili olabilece\u011fine inanmaktad\u0131r. Belirli bir a\u015famada aniden artan kozmik \u0131\u015f\u0131nlar\u0131n D\u00fcnya\u0027n\u0131n ozon tabakas\u0131na zarar verebilece\u011fini ve D\u00fcnya ortam\u0131n\u0131n radyoaktivitesini art\u0131rarak t\u00fcrlerin mutasyonuna ve hatta yok olmas\u0131na yol a\u00e7abilece\u011fini d\u00fc\u015f\u00fcn\u00fcyorlar. \u00d6te yandan, bu \u0131\u015f\u0131nlar yeni t\u00fcrlerin mutasyona u\u011framas\u0131n\u0131 te\u015fvik ederek tamamen yeni bir nesil yaratabilir. Bu teori ayn\u0131 zamanda, ma\u011faralarda, deniz dibinde veya yer alt\u0131nda ya\u015fayan baz\u0131 canl\u0131lar\u0131n tam da radyasyonun \u00e7o\u011fundan ka\u00e7abildikleri i\u00e7in yok olmad\u0131klar\u0131n\u0131 belirtmektedir. Bu a\u00e7\u0131dan bak\u0131ld\u0131\u011f\u0131nda, kozmik \u0131\u015f\u0131nlar ger\u00e7ekten de...", "type": "outside"}, {"angle": 0, "bbox": ["30", "641", "203", "670"], "bg_color": ["223", "223", "223"], "fg_color": ["133", "133", "133"], "fr": "...EN PARTICULES NEUTRES.", "id": "menjadi partikel netral.", "is_bold": false, "pt": "...PART\u00cdCULAS NEUTRAS.", "text": "into neutral particles.", "tr": "...n\u00f6tr par\u00e7ac\u0131klar haline gelir.", "type": "outside"}, {"angle": -0.12465175586390842, "bbox": ["16", "818", "439", "847"], "bg_color": ["197", "197", "197"], "fg_color": ["202", "202", "202"], "fr": "...DE V\u00c9RITABLES \"MISSILES COSMIQUES\"... ... ... ... ... ...", "id": "adalah \u0027rudal kosmik\u0027 yang sesungguhnya.........", "is_bold": false, "pt": "...VERDADEIROS \"M\u00cdSSEIS C\u00d3SMICOS\".........", "text": "the veritable \u0027cosmic missiles\u0027..........", "tr": "...tam anlam\u0131yla \u0027kozmik f\u00fczelerdir\u0027.........", "type": "outside"}, {"angle": -0.696788972861782, "bbox": ["437", "897", "901", "954"], "bg_color": ["47", "47", "47"], "fg_color": ["122", "122", "122"], "fr": "AVIS DE VACANCES DE LA F\u00caTE NATIONALE.", "id": "PENGUMUMAN LIBUR HARI NASIONAL", "is_bold": false, "pt": "AVISO DE FERIADO DO DIA NACIONAL", "text": "National Day Holiday Notice", "tr": "Ulusal G\u00fcn Tatil Bildirimi", "type": "outside"}], "width": 1080}, {"height": 454, "img_url": "snowmtl.ru/latest/the-original/205/13.webp", "translations": [{"angle": 0, "bbox": ["57", "18", "151", "151"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "QU\u0027EST-CE QUE VOUS FAITES, JE N\u0027AI PAS ENCORE FINI DE PARLER !", "id": "Hei, apa yang kalian lakukan, aku belum selesai bicara!", "is_bold": false, "pt": "O QUE VOC\u00caS EST\u00c3O FAZENDO? EU AINDA N\u00c3O TERMINEI DE FALAR!", "text": "What are you doing? I haven\u0027t finished talking yet!", "tr": "Ne yap\u0131yorsunuz, daha s\u00f6z\u00fcm\u00fc bitirmedim ki!", "type": "inside"}, {"angle": 0, "bbox": ["909", "37", "1029", "129"], "bg_color": ["255", "255", "255"], "fg_color": ["0", "0", "0"], "fr": "ALLEZ !", "id": "[SFX] BA!", "is_bold": false, "pt": "OK!", "text": "Ba!", "tr": "Haydi!", "type": "inside"}, {"angle": 0.10055126002379211, "bbox": ["184", "112", "288", "150"], "bg_color": ["217", "217", "217"], "fg_color": ["129", "129", "129"], "fr": "A\u00cfE !", "id": "Aduh!", "is_bold": false, "pt": "[SFX] AI!", "text": "Aiya!", "tr": "Aman!", "type": "sfx"}, {"angle": -0.0364642867797329, "bbox": ["239", "198", "318", "227"], "bg_color": ["191", "191", "191"], "fg_color": ["173", "173", "173"], "fr": "[SFX] AH !", "id": "[SFX] AHH!", "is_bold": false, "pt": "[SFX] AH!", "text": "Ah!", "tr": "Ah!", "type": "sfx"}, {"angle": -3.972754143456001, "bbox": ["534", "34", "888", "160"], "bg_color": ["141", "141", "141"], "fg_color": ["118", "118", "118"], "fr": "[SFX] PAF ! \u2661 AVIS DE NON-VACANCES POUR LA F\u00caTE NATIONALE.", "id": "\u2661 [SFX] PLAK! PENGUMUMAN TIDAK LIBUR NASIONAL", "is_bold": false, "pt": "\u2661 [SFX] PLAFT! AVISO: N\u00c3O HAVER\u00c1 FOLGA NO DIA NACIONAL", "text": "\u2661 SLAP!\nNational Day *No* Holiday Notice", "tr": "\u2661 [SFX] PAT! Ulusal G\u00fcn Tatil Yok Bildirimi", "type": "sfx"}, {"angle": 0.13688295580829504, "bbox": ["904", "159", "963", "197"], "bg_color": ["213", "213", "213"], "fg_color": ["128", "128", "128"], "fr": "...CORE !", "id": "Lho?", "is_bold": false, "pt": "HEIN?", "text": "...", "tr": "Ne yani?", "type": "outside"}, {"angle": -5.356066310469032e-06, "bbox": ["31", "379", "1030", "426"], "bg_color": ["162", "162", "162"], "fg_color": ["212", "212", "212"], "fr": "PAUSE DE MISE \u00c0 JOUR PENDANT LES VACANCES DE LA F\u00caTE NATIONALE, REPRISE LE 10 OCTOBRE. JOYEUSE F\u00caTE NATIONALE \u00c0 TOUS ~", "id": "Update dihentikan selama libur Hari Nasional, akan dilanjutkan pada 10 Oktober. Selamat Hari Nasional semuanya~", "is_bold": false, "pt": "PAUSA NAS ATUALIZA\u00c7\u00d5ES DURANTE O FERIADO DO DIA NACIONAL. AS ATUALIZA\u00c7\u00d5ES RETORNAM EM 10 DE OUTUBRO. FELIZ DIA NACIONAL A TODOS~", "text": "Updates will pause during the National Day holiday and resume on October 10th.\nWishing everyone a happy National Day~", "tr": "Ulusal G\u00fcn tatili boyunca yay\u0131n yok, 10 Ekim\u0027de g\u00fcncelleme olacak. Herkese mutlu Ulusal G\u00fcnler dilerim~", "type": "outside"}], "width": 1080}]

Manhua