. . "Astronomia de neutrinos \u00E9 o ramo da astronomia que observa objetos astron\u00F4micos, com detectores de neutrinos em especial observat\u00F3rios. Os neutrinos s\u00E3o criados como resultado de certos tipos de decaimento radioativo, ou rea\u00E7\u00F5es nucleares , tais como aqueles que ocorrem no Sol, em reatores nucleares, ou quando os raios c\u00F3smicos batem no \u00E1tomos. Devido \u00E0 sua fraca intera\u00E7\u00E3o com a mat\u00E9ria, os neutrinos oferecem uma oportunidade \u00FAnica para observar processos que s\u00E3o inacess\u00EDveis aos telesc\u00F3pios \u00F3pticos."@pt . . . . . . . "L\u2019astronomie neutrino (parfois astronomique neutrinique) est la branche de l'astronomie qui observe les objets c\u00E9lestes \u00E0 l'aide de d\u00E9tecteurs de neutrinos, des leptons neutres de faible masse d\u00E9crits par la th\u00E9orie \u00E9lectrofaible. \u00C9tant donn\u00E9 leur tr\u00E8s faible interaction avec la mati\u00E8re, les neutrinos ont la capacit\u00E9 de traverser des distances cosmologiques sans d\u00E9vier de leur trajectoire initiale, faisant d'eux d'excellents messagers astronomiques permettant de retracer directement l'origine de leur lieu de production."@fr . "\u041D\u0435\u0439\u0442\u0440\u0438\u043D\u043D\u0430 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0456\u044F \u2014 \u0433\u0430\u043B\u0443\u0437\u044C \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0456\u0457, \u0449\u043E \u0441\u043F\u043E\u0441\u0442\u0435\u0440\u0456\u0433\u0430\u0454 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0456\u0447\u043D\u0456 \u043E\u0431'\u0454\u043A\u0442\u0438 \u0432 \u0441\u043F\u0435\u0446\u0456\u0430\u043B\u044C\u043D\u0438\u0445 \u043E\u0431\u0441\u0435\u0440\u0432\u0430\u0442\u043E\u0440\u0456\u044F\u0445 \u0437\u0430 \u0434\u043E\u043F\u043E\u043C\u043E\u0433\u043E\u044E \u043D\u0435\u0439\u0442\u0440\u0438\u043D\u043D\u0438\u0445 \u0434\u0435\u0442\u0435\u043A\u0442\u043E\u0440\u0456\u0432. \u0427\u0430\u0441\u0442\u0438\u043D\u043A\u0438 \u043D\u0435\u0439\u0442\u0440\u0438\u043D\u043E \u0443\u0442\u0432\u043E\u0440\u044E\u044E\u0442\u044C\u0441\u044F \u0432\u043D\u0430\u0441\u043B\u0456\u0434\u043E\u043A \u0434\u0435\u044F\u043A\u0438\u0445 \u0432\u0438\u0434\u0456\u0432 \u0440\u0430\u0434\u0456\u043E\u0430\u043A\u0442\u0438\u0432\u043D\u043E\u0433\u043E \u0440\u043E\u0437\u043F\u0430\u0434\u0443, \u044F\u0434\u0435\u0440\u043D\u0438\u0445 \u0440\u0435\u0430\u043A\u0446\u0456\u0439, \u043F\u043E\u0434\u0456\u0431\u043D\u043E \u0434\u043E \u0442\u0438\u0445, \u0449\u043E \u0432\u0456\u0434\u0431\u0443\u0432\u0430\u044E\u0442\u044C\u0441\u044F \u043D\u0430 \u0421\u043E\u043D\u0446\u0456, \u0447\u0438 \u0432\u043D\u0430\u0441\u043B\u0456\u0434\u043E\u043A \u0437\u0456\u0442\u043A\u043D\u0435\u043D\u043D\u044F \u043A\u043E\u0441\u043C\u0456\u0447\u043D\u0438\u0445 \u043F\u0440\u043E\u043C\u0435\u043D\u0456\u0432 \u0437 \u0430\u0442\u043E\u043C\u0430\u043C\u0438. \u0427\u0435\u0440\u0435\u0437 \u0434\u0443\u0436\u0435 \u0441\u043B\u0430\u0431\u043A\u0443 \u0432\u0437\u0430\u0454\u043C\u043E\u0434\u0456\u044E \u0437 \u0440\u0435\u0447\u043E\u0432\u0438\u043D\u043E\u044E \u043D\u0435\u0439\u0442\u0440\u0438\u043D\u043E \u043D\u0430\u0434\u0430\u0454 \u0443\u043D\u0456\u043A\u0430\u043B\u044C\u043D\u0443 \u043C\u043E\u0436\u043B\u0438\u0432\u0456\u0441\u0442\u044C \u0441\u043F\u043E\u0441\u0442\u0435\u0440\u0456\u0433\u0430\u0442\u0438 \u0437\u0430 \u043F\u0440\u043E\u0446\u0435\u0441\u0430\u043C\u0438, \u044F\u043A\u0456 \u043D\u0435\u0434\u043E\u0441\u0442\u0443\u043F\u043D\u0456 \u0434\u043B\u044F \u043E\u043F\u0442\u0438\u0447\u043D\u0438\u0445 \u0442\u0435\u043B\u0435\u0441\u043A\u043E\u043F\u0456\u0432."@uk . . "R\u00E9alteola\u00EDocht neoidr\u00EDon\u00F3"@ga . "\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u5B66\uFF08\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u3066\u3093\u3082\u3093\u304C\u304F\u3001\u82F1: neutrino astronomy\uFF09\u306F\u3001\u5929\u6587\u5B66\u306E\u4E00\u5206\u91CE\u3002\u592A\u967D\u3084\u8D85\u65B0\u661F\u7206\u767A\u3067\u751F\u6210\u3055\u308C\u308B\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u3092\u89B3\u6E2C\u3057\u3001\u5929\u6587\u73FE\u8C61\u306E\u89E3\u660E\u306B\u5F79\u7ACB\u3066\u308B\u3053\u3068\u3092\u76EE\u7684\u3068\u3059\u308B\u3002\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u5B66\u306F\u307E\u3060\u767A\u5C55\u9014\u4E0A\u306E\u5206\u91CE\u3067\u3042\u308A\u3001\u78BA\u8A8D\u3055\u308C\u3066\u3044\u308B\u5730\u7403\u5916\u306E\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u6E90\u306F\u592A\u967D\u3068\u8D85\u65B0\u661FSN 1987A\u306E\u307F\u3067\u3042\u308B\u3002 \u89B3\u6E2C\u88C5\u7F6E\u3068\u3057\u3066\u306F\u30AB\u30DF\u30AA\u30AB\u30F3\u30C7\uFF08\u89E3\u4F53\u6E08\u307F\uFF09\u3001\u30B9\u30FC\u30D1\u30FC\u30AB\u30DF\u30AA\u30AB\u30F3\u30C7\u3001\u30AB\u30E0\u30E9\u30F3\u30C9\u3001\u30B5\u30C9\u30D9\u30EA\u30FC\u30FB\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u53F0 (SNO)\u3001ANTARES\u3001\u3001\u30A2\u30A4\u30B9\u30AD\u30E5\u30FC\u30D6\u306A\u3069\u304C\u3042\u308B\u3002 \u6771\u4EAC\u5927\u5B66\u540D\u8A89\u6559\u6388\u306E\u5C0F\u67F4\u660C\u4FCA\u3001\u30DA\u30F3\u30B7\u30EB\u30D9\u30CB\u30A2\u5927\u5B66\u540D\u8A89\u6559\u6388\u306E\u30EC\u30A4\u30E2\u30F3\u30C9\u30FB\u30C7\u30FC\u30D3\u30B9\u304C\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u5B66\u306E\u3055\u304D\u304C\u3051\u3068\u306A\u308B\u6210\u679C\u3092\u3042\u3052\u305F\u3068\u3057\u3066\u30012002\u5E74\u306B\u30CE\u30FC\u30D9\u30EB\u7269\u7406\u5B66\u8CDE\u3092\u53D7\u8CDE\u3057\u305F\u3002"@ja . . . . . . . . "Astronomia de neutrinos"@pt . . . "Neutrinov\u00E1 astronomie je odv\u011Btv\u00ED astronomie zab\u00FDvaj\u00EDc\u00ED a zkoumaj\u00EDc\u00ED astronomick\u00E9 objekty pomoc\u00ED neutrinov\u00FDch detektor\u016F ve specializovan\u00FDch observato\u0159\u00EDch. Jadern\u00E9 reakce uvnit\u0159 hv\u011Bzd a exploze supernov produkuj\u00ED obrovsk\u00E1 mno\u017Estv\u00ED neutrin, z nich\u017E jen velmi mal\u00E9 mno\u017Estv\u00ED m\u016F\u017Ee b\u00FDt odhaleno pomoc\u00ED tzv. neutrinov\u00FDch teleskop\u016F. Hlavn\u00ED motivac\u00ED neutrinov\u00E9 astronomie je mo\u017Enost pozorovat procesy, kter\u00E9 jsou b\u011B\u017En\u00FDm optick\u00FDm teleskop\u016Fm nedostupn\u00E9 jako nap\u0159. slune\u010Dn\u00ED j\u00E1dro. Neutrinov\u00E1 astronomie je st\u00E1le v ran\u00E9 f\u00E1zi sv\u00E9ho v\u00FDvoje a jako jedin\u00E9 doposud potvrzen\u00E9 mimozemsk\u00E9 zdroje neutrin byly potvrzeny Slunce a supernova SN 1987A."@cs . . . "\u041D\u0435\u0439\u0442\u0440\u0438\u0301\u043D\u043D\u0430\u044F \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u0301\u043C\u0438\u044F \u2014 \u0440\u0430\u0437\u0434\u0435\u043B \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0438, \u0438\u0437\u0443\u0447\u0430\u044E\u0449\u0438\u0439 \u043D\u0435\u0439\u0442\u0440\u0438\u043D\u043D\u043E\u0435 \u0438\u0437\u043B\u0443\u0447\u0435\u043D\u0438\u0435 \u0432\u043D\u0435\u0437\u0435\u043C\u043D\u044B\u0445 \u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u043E\u0432 \u0441 \u0446\u0435\u043B\u044C\u044E \u043F\u043E\u043B\u0443\u0447\u0435\u043D\u0438\u044F \u0441\u0432\u0435\u0434\u0435\u043D\u0438\u0439 \u043E \u043F\u0440\u043E\u0438\u0441\u0445\u043E\u0434\u044F\u0449\u0438\u0445 \u0432 \u043A\u043E\u0441\u043C\u043E\u0441\u0435 \u043F\u0440\u043E\u0446\u0435\u0441\u0441\u0430\u0445."@ru . "Astronomia neutrinowa \u2013 ga\u0142\u0105\u017A astronomii, w kt\u00F3rej obserwacje obiekt\u00F3w na niebie prowadzi si\u0119 poprzez detekcj\u0119 neutrin, emitowanych przez te cia\u0142a niebieskie. Neutrina produkowane s\u0105 we wn\u0119trzach gwiazd, w szczeg\u00F3lno\u015Bci w czasie wybuchu supernowej. Ich \u017Ar\u00F3d\u0142em s\u0105 zachodz\u0105ce tam reakcje termoj\u0105drowe. Astronomia neutrinowa daje mo\u017Cliwo\u015B\u0107 obserwacji obszar\u00F3w nieobserwowalnych przez jakiekolwiek teleskopy, nie tylko optyczne. Astronomia ta jest na pocz\u0105tku swego rozwoju i jak dotychczas zarejestrowano tylko dwa kosmiczne \u017Ar\u00F3d\u0142a neutrin: S\u0142o\u0144ce oraz supernow\u0105 SN 1987A. Obserwacje S\u0142o\u0144ca w zakresie neutrin w decyduj\u0105cej mierze przyczyni\u0142y si\u0119 do prze\u0142omowego dla fizyki odkrycia oscylacji neutrin."@pl . "\u041D\u0435\u0439\u0442\u0440\u0438\u0301\u043D\u043D\u0430\u044F \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u0301\u043C\u0438\u044F \u2014 \u0440\u0430\u0437\u0434\u0435\u043B \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0438, \u0438\u0437\u0443\u0447\u0430\u044E\u0449\u0438\u0439 \u043D\u0435\u0439\u0442\u0440\u0438\u043D\u043D\u043E\u0435 \u0438\u0437\u043B\u0443\u0447\u0435\u043D\u0438\u0435 \u0432\u043D\u0435\u0437\u0435\u043C\u043D\u044B\u0445 \u0438\u0441\u0442\u043E\u0447\u043D\u0438\u043A\u043E\u0432 \u0441 \u0446\u0435\u043B\u044C\u044E \u043F\u043E\u043B\u0443\u0447\u0435\u043D\u0438\u044F \u0441\u0432\u0435\u0434\u0435\u043D\u0438\u0439 \u043E \u043F\u0440\u043E\u0438\u0441\u0445\u043E\u0434\u044F\u0449\u0438\u0445 \u0432 \u043A\u043E\u0441\u043C\u043E\u0441\u0435 \u043F\u0440\u043E\u0446\u0435\u0441\u0441\u0430\u0445."@ru . . . . . . . "1121960724"^^ . "Neutrinoastronomi \u00E4r ett nytt f\u00F6nster mot universum, som g\u00E5r ut p\u00E5 att studera dels de v\u00E4ldiga fl\u00F6den av neutriner som n\u00E5r oss fr\u00E5n stj\u00E4rnor i olika stadier av sina livscykler, dels en trolig bakgrundsstr\u00E5lning av samma ursprung som den elektromagnetiska. Denna vetenskap \u00E4r fortfarande i sin linda \u2013 de enda hittills bekr\u00E4ftade utomjordiska k\u00E4llorna \u00E4r solen och supernovan SN 1987A. Sv\u00E5righeten ligger i att \u00F6ver huvud taget kunna detektera neutrinerna, som n\u00E4stan inte alls v\u00E4xelverkar med vanlig materia. Att kunna observera astronomiska fenomen i \u201Dljuset\u201D av neutriner \u00E4r trots allt en tillr\u00E4ckligt lovande informationsk\u00E4lla f\u00F6r att motivera stora anstr\u00E4ngningar f\u00F6r att utveckla fungerande detekteringssystem."@sv . . "Iarrachta\u00ED neoidr\u00EDon\u00F3nna \u00F3n nGrian a bhrath chun na coinn\u00EDollacha i gcro\u00EDleac\u00E1n soladach na Gr\u00E9ine a dh\u00E9anamh amach, agus mar an gc\u00E9anna maidir le holln\u00F3va\u00ED. De r\u00E9ir na dturgnamh \u00F3 na 1960id\u00ED, t\u00E1 r\u00E1ta sreafa na neoidr\u00EDon\u00F3nna grianda n\u00EDos l\u00FA n\u00E1 mar a bh\u00EDodh \u00E1 thuar \u00F3 theoiric na n\u00FAicl\u00E9isint\u00E9ise."@ga . . "Astronomia neutrinowa"@pl . . "L'astronomia dei neutrini \u00E8 quella branca dell'astronomia che osserva gli oggetti astronomici tramite rivelatori di neutrini in speciali osservatori. Le reazioni di fusione nucleare all'interno delle stelle e le esplosioni delle supernovae producono grandi quantit\u00E0 di neutrini, dei quali solo una minima parte pu\u00F2 tuttavia essere misurata. L'astronomia dei neutrini trova il suo impiego principale nella possibilit\u00E0 di osservare processi e strutture inaccessibili alle normali attrezzature ottiche, come i fenomeni nucleari nel nucleo solare."@it . . . . . . . "33718"^^ . . . . . . "Neutrino astronomy is the branch of astronomy that observes astronomical objects with neutrino detectors in special observatories. Neutrinos are created as a result of certain types of radioactive decay, nuclear reactions such as those that take place in the Sun or high energy astrophysical phenomena, in nuclear reactors, or when cosmic rays hit atoms in the atmosphere. Neutrinos rarely interact with matter, meaning that it is unlikely for them to scatter along their trajectory, unlike photons. Therefore, neutrinos offer a unique opportunity to observe processes that are inaccessible to optical telescopes, such as reactions in the Sun's core. Neutrinos can also offer a very strong pointing direction compared to charged particle cosmic rays."@en . "Neutrinoastronomi"@sv . . . . . . . . . . . "Neutrinov\u00E1 astronomie je odv\u011Btv\u00ED astronomie zab\u00FDvaj\u00EDc\u00ED a zkoumaj\u00EDc\u00ED astronomick\u00E9 objekty pomoc\u00ED neutrinov\u00FDch detektor\u016F ve specializovan\u00FDch observato\u0159\u00EDch. Jadern\u00E9 reakce uvnit\u0159 hv\u011Bzd a exploze supernov produkuj\u00ED obrovsk\u00E1 mno\u017Estv\u00ED neutrin, z nich\u017E jen velmi mal\u00E9 mno\u017Estv\u00ED m\u016F\u017Ee b\u00FDt odhaleno pomoc\u00ED tzv. neutrinov\u00FDch teleskop\u016F. Hlavn\u00ED motivac\u00ED neutrinov\u00E9 astronomie je mo\u017Enost pozorovat procesy, kter\u00E9 jsou b\u011B\u017En\u00FDm optick\u00FDm teleskop\u016Fm nedostupn\u00E9 jako nap\u0159. slune\u010Dn\u00ED j\u00E1dro."@cs . "Astronomi neutrino adalah cabang astronomi yang mengamati benda-benda langit dengan menggunakan di observatorium khusus. Neutrino terbuat dari peluruhan radioaktif jenis tertentu atau reaksi nuklir seperti yang terjadi di dalam Matahari, di dalam reaktor nuklir, atau saat sinar kosmis menghujam atom. Neutrino memiliki interaksi yang lemah dengan materi dan dapat melewatinya nyaris tanpa halangan, sehingga dapat dimanfaatkan untuk mengamati proses-proses yang tidak dapat dilihat dengan menggunakan teleskop optik."@in . . . . . . . "\uC911\uC131\uBBF8\uC790 \uCC9C\uBB38\uD559"@ko . . "Astronomia neutrinowa \u2013 ga\u0142\u0105\u017A astronomii, w kt\u00F3rej obserwacje obiekt\u00F3w na niebie prowadzi si\u0119 poprzez detekcj\u0119 neutrin, emitowanych przez te cia\u0142a niebieskie. Neutrina produkowane s\u0105 we wn\u0119trzach gwiazd, w szczeg\u00F3lno\u015Bci w czasie wybuchu supernowej. Ich \u017Ar\u00F3d\u0142em s\u0105 zachodz\u0105ce tam reakcje termoj\u0105drowe. Astronomia neutrinowa daje mo\u017Cliwo\u015B\u0107 obserwacji obszar\u00F3w nieobserwowalnych przez jakiekolwiek teleskopy, nie tylko optyczne. Astronomia ta jest na pocz\u0105tku swego rozwoju i jak dotychczas zarejestrowano tylko dwa kosmiczne \u017Ar\u00F3d\u0142a neutrin: S\u0142o\u0144ce oraz supernow\u0105 SN 1987A."@pl . "Neutrinoastronomi \u00E4r ett nytt f\u00F6nster mot universum, som g\u00E5r ut p\u00E5 att studera dels de v\u00E4ldiga fl\u00F6den av neutriner som n\u00E5r oss fr\u00E5n stj\u00E4rnor i olika stadier av sina livscykler, dels en trolig bakgrundsstr\u00E5lning av samma ursprung som den elektromagnetiska. Denna vetenskap \u00E4r fortfarande i sin linda \u2013 de enda hittills bekr\u00E4ftade utomjordiska k\u00E4llorna \u00E4r solen och supernovan SN 1987A. Sv\u00E5righeten ligger i att \u00F6ver huvud taget kunna detektera neutrinerna, som n\u00E4stan inte alls v\u00E4xelverkar med vanlig materia. Att kunna observera astronomiska fenomen i \u201Dljuset\u201D av neutriner \u00E4r trots allt en tillr\u00E4ckligt lovande informationsk\u00E4lla f\u00F6r att motivera stora anstr\u00E4ngningar f\u00F6r att utveckla fungerande detekteringssystem."@sv . . "\uC911\uC131\uBBF8\uC790 \uCC9C\uBB38\uD559(\uC601\uC5B4: Neutrino astronomy)\uC740 \uB97C \uC774\uC6A9\uD574 \uCC9C\uCCB4\uB97C \uAD00\uCE21\uD558\uB294 \uAC83\uC744 \uB9D0\uD55C\uB2E4. \uC911\uC131\uBBF8\uC790\uB294 \uBC29\uC0AC\uC131 \uBD95\uAD34, \uD0DC\uC591\uACFC \uC6D0\uC790\uB85C\uC5D0\uC11C \uC77C\uC5B4\uB098\uB294 \uD575\uBC18\uC751, \uC6B0\uC8FC\uC120\uC774 \uC6D0\uC790\uC640 \uCDA9\uB3CC\uD560 \uB54C \uC8FC\uB85C \uBC1C\uC0DD\uD558\uBA70, \uBB3C\uC9C8\uACFC\uC758 \uC0C1\uD638\uC791\uC6A9\uC774 \uC801\uAE30 \uB54C\uBB38\uC5D0 \uAD11\uD559 \uB9DD\uC6D0\uACBD\uC73C\uB85C \uAD00\uCE21\uD560 \uC218 \uC5C6\uB294 \uAC83\uC744 \uAD00\uCE21\uD560 \uC218 \uC788\uAC8C \uD574 \uC8FC\uAE30\uB3C4 \uD55C\uB2E4."@ko . . "L\u2019astronomie neutrino (parfois astronomique neutrinique) est la branche de l'astronomie qui observe les objets c\u00E9lestes \u00E0 l'aide de d\u00E9tecteurs de neutrinos, des leptons neutres de faible masse d\u00E9crits par la th\u00E9orie \u00E9lectrofaible. \u00C9tant donn\u00E9 leur tr\u00E8s faible interaction avec la mati\u00E8re, les neutrinos ont la capacit\u00E9 de traverser des distances cosmologiques sans d\u00E9vier de leur trajectoire initiale, faisant d'eux d'excellents messagers astronomiques permettant de retracer directement l'origine de leur lieu de production. L'observation de neutrinos cosmiques permet de mieux \u00E9tudier le fonctionnement des ph\u00E9nom\u00E8nes les plus \u00E9nerg\u00E9tiques et les plus \u00E9loign\u00E9s de l'Univers. Toutefois, la difficult\u00E9 de d\u00E9tecter ces particules limite \u00E0 ce jour la capacit\u00E9 de d\u00E9tection d'objets c\u00E9lestes \u00E9mettant des neutrinos. Avant 2022, seules trois associations de neutrinos \u00E0 des objets c\u00E9lestes ont pu \u00EAtre \u00E9tablies: le Soleil, la supernova 1987A, ainsi que la galaxie active TXS0506+056."@fr . . . 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"Iarrachta\u00ED neoidr\u00EDon\u00F3nna \u00F3n nGrian a bhrath chun na coinn\u00EDollacha i gcro\u00EDleac\u00E1n soladach na Gr\u00E9ine a dh\u00E9anamh amach, agus mar an gc\u00E9anna maidir le holln\u00F3va\u00ED. De r\u00E9ir na dturgnamh \u00F3 na 1960id\u00ED, t\u00E1 r\u00E1ta sreafa na neoidr\u00EDon\u00F3nna grianda n\u00EDos l\u00FA n\u00E1 mar a bh\u00EDodh \u00E1 thuar \u00F3 theoiric na n\u00FAicl\u00E9isint\u00E9ise."@ga . "L'astronomia dei neutrini \u00E8 quella branca dell'astronomia che osserva gli oggetti astronomici tramite rivelatori di neutrini in speciali osservatori. Le reazioni di fusione nucleare all'interno delle stelle e le esplosioni delle supernovae producono grandi quantit\u00E0 di neutrini, dei quali solo una minima parte pu\u00F2 tuttavia essere misurata. L'astronomia dei neutrini trova il suo impiego principale nella possibilit\u00E0 di osservare processi e strutture inaccessibili alle normali attrezzature ottiche, come i fenomeni nucleari nel nucleo solare."@it . "\u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u064A\u0646\u0648 \u0647\u0648 \u0641\u0631\u0639 \u0645\u0646 \u0641\u0631\u0648\u0639 \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0630\u064A \u064A\u062F\u0631\u0633 \u0627\u0644\u0623\u062C\u0631\u0627\u0645 \u0627\u0644\u0641\u0644\u0643\u064A\u0629 \u0628\u0648\u0627\u0633\u0637\u0629 \u0623\u062C\u0647\u0632\u0629 \u0627\u0644\u0643\u0634\u0641 \u0639\u0646 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u064A\u0646\u0648 \u0641\u064A \u0627\u0644\u0645\u0631\u0627\u0635\u062F \u0627\u0644\u062E\u0627\u0635\u0629. \u062A\u0646\u0634\u0623 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u064A\u0646\u0648\u0627\u062A \u0646\u062A\u064A\u062C\u0629 \u0644\u0623\u0646\u0648\u0627\u0639 \u0645\u0639\u064A\u0646\u0629 \u0645\u0646 \u0627\u0644\u0627\u0636\u0645\u062D\u0644\u0627\u0644 \u0627\u0644\u0625\u0634\u0639\u0627\u0639\u064A\u060C \u0623\u0648 \u0627\u0644\u062A\u0641\u0627\u0639\u0644\u0627\u062A \u0627\u0644\u0646\u0648\u0648\u064A\u0629 \u0645\u062B\u0644 \u062A\u0644\u0643 \u0627\u0644\u062A\u064A \u062A\u062D\u062F\u062B \u0641\u064A \u0627\u0644\u0634\u0645\u0633 \u0623\u0648 \u0641\u064A \u0627\u0644\u0645\u0641\u0627\u0639\u0644\u0627\u062A \u0627\u0644\u0646\u0648\u0648\u064A\u0629 \u0623\u0648 \u0639\u0646\u062F\u0645\u0627 \u062A\u0635\u064A\u0628 \u0627\u0644\u0623\u0634\u0639\u0629 \u0627\u0644\u0643\u0648\u0646\u064A\u0629 \u0627\u0644\u0630\u0631\u0627\u062A. \u0628\u0633\u0628\u0628 \u062A\u0641\u0627\u0639\u0644\u0627\u062A\u0647\u0627 \u0627\u0644\u0636\u0639\u064A\u0641\u0629 \u0645\u0639 \u0627\u0644\u0645\u0627\u062F\u0629\u060C \u062A\u0648\u0641\u0631 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u064A\u0646\u0648\u0627\u062A \u0641\u0631\u0635\u0629 \u0641\u0631\u064A\u062F\u0629 \u0644\u0645\u0631\u0627\u0642\u0628\u0629 \u0627\u0644\u0639\u0645\u0644\u064A\u0627\u062A \u0627\u0644\u062A\u064A \u062A\u062D\u062F\u062B \u0628\u0627\u0644\u0641\u0636\u0627\u0621 \u0648\u0627\u0644\u062A\u064A \u064A\u062A\u0639\u0630\u0631 \u0627\u0644\u0648\u0635\u0648\u0644 \u0625\u0644\u064A\u0647\u0627 \u0628\u0627\u0644\u062A\u0644\u0633\u0643\u0648\u0628\u0627\u062A \u0627\u0644\u0628\u0635\u0631\u064A\u0629."@ar . . . "Astronomi neutrino"@in . . . "Astronomia de neutrinos \u00E9 o ramo da astronomia que observa objetos astron\u00F4micos, com detectores de neutrinos em especial observat\u00F3rios. Os neutrinos s\u00E3o criados como resultado de certos tipos de decaimento radioativo, ou rea\u00E7\u00F5es nucleares , tais como aqueles que ocorrem no Sol, em reatores nucleares, ou quando os raios c\u00F3smicos batem no \u00E1tomos. Devido \u00E0 sua fraca intera\u00E7\u00E3o com a mat\u00E9ria, os neutrinos oferecem uma oportunidade \u00FAnica para observar processos que s\u00E3o inacess\u00EDveis aos telesc\u00F3pios \u00F3pticos."@pt . "La astronom\u00EDa de neutrinos es la ciencia de observar fen\u00F3menos astron\u00F3micos detectando neutrinos. Estos neutrinos son un producto de las reacciones termonucleares d\u00E9biles que tienen lugar en el interior de cada estrella.\u200B"@es . "Neutrino astronomy"@en . . "\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u5B66\uFF08\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u3066\u3093\u3082\u3093\u304C\u304F\u3001\u82F1: neutrino astronomy\uFF09\u306F\u3001\u5929\u6587\u5B66\u306E\u4E00\u5206\u91CE\u3002\u592A\u967D\u3084\u8D85\u65B0\u661F\u7206\u767A\u3067\u751F\u6210\u3055\u308C\u308B\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u3092\u89B3\u6E2C\u3057\u3001\u5929\u6587\u73FE\u8C61\u306E\u89E3\u660E\u306B\u5F79\u7ACB\u3066\u308B\u3053\u3068\u3092\u76EE\u7684\u3068\u3059\u308B\u3002\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u5B66\u306F\u307E\u3060\u767A\u5C55\u9014\u4E0A\u306E\u5206\u91CE\u3067\u3042\u308A\u3001\u78BA\u8A8D\u3055\u308C\u3066\u3044\u308B\u5730\u7403\u5916\u306E\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u6E90\u306F\u592A\u967D\u3068\u8D85\u65B0\u661FSN 1987A\u306E\u307F\u3067\u3042\u308B\u3002 \u89B3\u6E2C\u88C5\u7F6E\u3068\u3057\u3066\u306F\u30AB\u30DF\u30AA\u30AB\u30F3\u30C7\uFF08\u89E3\u4F53\u6E08\u307F\uFF09\u3001\u30B9\u30FC\u30D1\u30FC\u30AB\u30DF\u30AA\u30AB\u30F3\u30C7\u3001\u30AB\u30E0\u30E9\u30F3\u30C9\u3001\u30B5\u30C9\u30D9\u30EA\u30FC\u30FB\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u53F0 (SNO)\u3001ANTARES\u3001\u3001\u30A2\u30A4\u30B9\u30AD\u30E5\u30FC\u30D6\u306A\u3069\u304C\u3042\u308B\u3002 \u6771\u4EAC\u5927\u5B66\u540D\u8A89\u6559\u6388\u306E\u5C0F\u67F4\u660C\u4FCA\u3001\u30DA\u30F3\u30B7\u30EB\u30D9\u30CB\u30A2\u5927\u5B66\u540D\u8A89\u6559\u6388\u306E\u30EC\u30A4\u30E2\u30F3\u30C9\u30FB\u30C7\u30FC\u30D3\u30B9\u304C\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u5B66\u306E\u3055\u304D\u304C\u3051\u3068\u306A\u308B\u6210\u679C\u3092\u3042\u3052\u305F\u3068\u3057\u3066\u30012002\u5E74\u306B\u30CE\u30FC\u30D9\u30EB\u7269\u7406\u5B66\u8CDE\u3092\u53D7\u8CDE\u3057\u305F\u3002"@ja . "\uC911\uC131\uBBF8\uC790 \uCC9C\uBB38\uD559(\uC601\uC5B4: Neutrino astronomy)\uC740 \uB97C \uC774\uC6A9\uD574 \uCC9C\uCCB4\uB97C \uAD00\uCE21\uD558\uB294 \uAC83\uC744 \uB9D0\uD55C\uB2E4. \uC911\uC131\uBBF8\uC790\uB294 \uBC29\uC0AC\uC131 \uBD95\uAD34, \uD0DC\uC591\uACFC \uC6D0\uC790\uB85C\uC5D0\uC11C \uC77C\uC5B4\uB098\uB294 \uD575\uBC18\uC751, \uC6B0\uC8FC\uC120\uC774 \uC6D0\uC790\uC640 \uCDA9\uB3CC\uD560 \uB54C \uC8FC\uB85C \uBC1C\uC0DD\uD558\uBA70, \uBB3C\uC9C8\uACFC\uC758 \uC0C1\uD638\uC791\uC6A9\uC774 \uC801\uAE30 \uB54C\uBB38\uC5D0 \uAD11\uD559 \uB9DD\uC6D0\uACBD\uC73C\uB85C \uAD00\uCE21\uD560 \uC218 \uC5C6\uB294 \uAC83\uC744 \uAD00\uCE21\uD560 \uC218 \uC788\uAC8C \uD574 \uC8FC\uAE30\uB3C4 \uD55C\uB2E4."@ko . "\u30CB\u30E5\u30FC\u30C8\u30EA\u30CE\u5929\u6587\u5B66"@ja . . "\u4E2D\u5FAE\u5B50\u5929\u6587\u5B66\u4EE5\u6D4B\u91CF\u4E2D\u5FAE\u5B50\u7684\u6D41\u91CF\u4E3A\u4E3B\u8981\u624B\u6BB5\uFF0C\u7814\u7A76\u5929\u4F53\u7269\u7406\u8FC7\u7A0B\u3002\u6052\u661F\u5185\u90E8\u7684\u6838\u53CD\u5E94\u3001\u8D85\u65B0\u661F\u7206\u53D1\u7B49\u8FC7\u7A0B\u90FD\u4F1A\u53D1\u51FA\u5927\u91CF\u7684\u4E2D\u5FAE\u5B50\u3002\u4E2D\u5FAE\u5B50\u662F\u4E00\u79CD\u8F7B\u5B50\uFF0C\u4E0D\u53C2\u4E0E\u5F3A\u76F8\u4E92\u4F5C\u7528\u548C\u7535\u78C1\u76F8\u4E92\u4F5C\u7528\uFF0C\u4E0E\u666E\u901A\u7269\u8D28\u7684\u53CD\u5E94\u622A\u9762\u5F88\u5C0F\uFF0C\u5E73\u5747\u81EA\u7531\u7A0B\u5F88\u957F\uFF0C\u7ED9\u63A2\u6D4B\u5E26\u6765\u4E86\u5F88\u5927\u7684\u56F0\u96BE\u3002\u592A\u9633\u4E2D\u5FAE\u5B50\u662F\u5728\u592A\u9633\u5185\u90E8\u6838\u53CD\u5E94\u8FC7\u7A0B\u4E2D\u4EA7\u751F\u7684\uFF0C\u5728\u5730\u7403\u9644\u8FD1\u5177\u6709\u5F88\u9AD8\u7684\u6D41\u91CF\u3002\u56E0\u4E3A\u4E2D\u5FAE\u5B50\u4E0E\u7269\u8D28\u7684\u5F31\u76F8\u4E92\u4F5C\u7528\uFF0C\u4E2D\u5FAE\u5B50\u63D0\u4F9B\u4E86\u4E00\u4E2A\u72EC\u7279\u7684\u673A\u4F1A\u53BB\u89C2\u5BDF\u90A3\u4E9B\u5149\u5B66\u671B\u8FDC\u955C\u65E0\u6CD5\u63A5\u89E6\u7684\u8FC7\u7A0B\u3002 \u4E2D\u5FAE\u5B50\u5929\u6587\u5B66\u9886\u57DF\u4ECD\u7136\u5904\u4E8E\u975E\u5E38\u521D\u671F\u7684\u9636\u6BB5 - \u552F\u4E00\u8BC1\u5B9E\u5730\u7403\u4E4B\u5916\u6765\u6E90\u81F3\u4ECA\u4E3A\u6B62\u4EC5\u6709\u592A\u9633\u548C\u8D85\u65B0\u661FSN 1987A\u3002"@zh . . . . . . . . . . . . . . . . . . "La astronom\u00EDa de neutrinos es la ciencia de observar fen\u00F3menos astron\u00F3micos detectando neutrinos. Estos neutrinos son un producto de las reacciones termonucleares d\u00E9biles que tienen lugar en el interior de cada estrella.\u200B"@es . . . . . . . "\u0639\u0644\u0645 \u0641\u0644\u0643 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u064A\u0646\u0648"@ar . "Astronomie neutrino"@fr . . "\u4E2D\u5FAE\u5B50\u5929\u6587\u5B66\u4EE5\u6D4B\u91CF\u4E2D\u5FAE\u5B50\u7684\u6D41\u91CF\u4E3A\u4E3B\u8981\u624B\u6BB5\uFF0C\u7814\u7A76\u5929\u4F53\u7269\u7406\u8FC7\u7A0B\u3002\u6052\u661F\u5185\u90E8\u7684\u6838\u53CD\u5E94\u3001\u8D85\u65B0\u661F\u7206\u53D1\u7B49\u8FC7\u7A0B\u90FD\u4F1A\u53D1\u51FA\u5927\u91CF\u7684\u4E2D\u5FAE\u5B50\u3002\u4E2D\u5FAE\u5B50\u662F\u4E00\u79CD\u8F7B\u5B50\uFF0C\u4E0D\u53C2\u4E0E\u5F3A\u76F8\u4E92\u4F5C\u7528\u548C\u7535\u78C1\u76F8\u4E92\u4F5C\u7528\uFF0C\u4E0E\u666E\u901A\u7269\u8D28\u7684\u53CD\u5E94\u622A\u9762\u5F88\u5C0F\uFF0C\u5E73\u5747\u81EA\u7531\u7A0B\u5F88\u957F\uFF0C\u7ED9\u63A2\u6D4B\u5E26\u6765\u4E86\u5F88\u5927\u7684\u56F0\u96BE\u3002\u592A\u9633\u4E2D\u5FAE\u5B50\u662F\u5728\u592A\u9633\u5185\u90E8\u6838\u53CD\u5E94\u8FC7\u7A0B\u4E2D\u4EA7\u751F\u7684\uFF0C\u5728\u5730\u7403\u9644\u8FD1\u5177\u6709\u5F88\u9AD8\u7684\u6D41\u91CF\u3002\u56E0\u4E3A\u4E2D\u5FAE\u5B50\u4E0E\u7269\u8D28\u7684\u5F31\u76F8\u4E92\u4F5C\u7528\uFF0C\u4E2D\u5FAE\u5B50\u63D0\u4F9B\u4E86\u4E00\u4E2A\u72EC\u7279\u7684\u673A\u4F1A\u53BB\u89C2\u5BDF\u90A3\u4E9B\u5149\u5B66\u671B\u8FDC\u955C\u65E0\u6CD5\u63A5\u89E6\u7684\u8FC7\u7A0B\u3002 \u4E2D\u5FAE\u5B50\u5929\u6587\u5B66\u9886\u57DF\u4ECD\u7136\u5904\u4E8E\u975E\u5E38\u521D\u671F\u7684\u9636\u6BB5 - \u552F\u4E00\u8BC1\u5B9E\u5730\u7403\u4E4B\u5916\u6765\u6E90\u81F3\u4ECA\u4E3A\u6B62\u4EC5\u6709\u592A\u9633\u548C\u8D85\u65B0\u661FSN 1987A\u3002"@zh . . "Neutrino astronomy is the branch of astronomy that observes astronomical objects with neutrino detectors in special observatories. Neutrinos are created as a result of certain types of radioactive decay, nuclear reactions such as those that take place in the Sun or high energy astrophysical phenomena, in nuclear reactors, or when cosmic rays hit atoms in the atmosphere. Neutrinos rarely interact with matter, meaning that it is unlikely for them to scatter along their trajectory, unlike photons. Therefore, neutrinos offer a unique opportunity to observe processes that are inaccessible to optical telescopes, such as reactions in the Sun's core. Neutrinos can also offer a very strong pointing direction compared to charged particle cosmic rays. Since neutrinos interact weakly, neutrino detectors must have large target masses (often thousands of tons). The detectors also must use shielding and effective software to remove background signal."@en . "\u041D\u0435\u0439\u0442\u0440\u0438\u043D\u043D\u0430\u044F \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u044F"@ru . . . . . . "Astronomia dei neutrini"@it . . . . "633325"^^ . . "Astronom\u00EDa de neutrinos"@es . "\u5FAE\u4E2D\u5B50\u5929\u6587\u5B66"@zh . . . . . "Astronomi neutrino adalah cabang astronomi yang mengamati benda-benda langit dengan menggunakan di observatorium khusus. Neutrino terbuat dari peluruhan radioaktif jenis tertentu atau reaksi nuklir seperti yang terjadi di dalam Matahari, di dalam reaktor nuklir, atau saat sinar kosmis menghujam atom. Neutrino memiliki interaksi yang lemah dengan materi dan dapat melewatinya nyaris tanpa halangan, sehingga dapat dimanfaatkan untuk mengamati proses-proses yang tidak dapat dilihat dengan menggunakan teleskop optik."@in . . . . "Neutrinov\u00E1 astronomie"@cs . .