| dbo:abstract |
الأشعة الكونية من خارج المجرة هي جزيئات عالية الطاقة تدخل إلى المجموعة الشمسية من خارج مجرة درب التبانة. تزيد الطاقة التي تمتلكها هذه الجسيمات عن 〖10〗^15 إلكترون فولت. (ar) Extragalactic cosmic rays are very-high-energy particles that flow into the Solar System from beyond the Milky Way galaxy. While at low energies, the majority of cosmic rays originate within the Galaxy (such as from supernova remnants), at high energies the cosmic ray spectrum is dominated by these extragalactic cosmic rays. The exact energy at which the transition from galactic to extragalactic cosmic rays occurs is not clear, but it is in the range 1017 to 1018 eV. (en) |
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| rdfs:comment |
الأشعة الكونية من خارج المجرة هي جزيئات عالية الطاقة تدخل إلى المجموعة الشمسية من خارج مجرة درب التبانة. تزيد الطاقة التي تمتلكها هذه الجسيمات عن 〖10〗^15 إلكترون فولت. (ar) Extragalactic cosmic rays are very-high-energy particles that flow into the Solar System from beyond the Milky Way galaxy. While at low energies, the majority of cosmic rays originate within the Galaxy (such as from supernova remnants), at high energies the cosmic ray spectrum is dominated by these extragalactic cosmic rays. The exact energy at which the transition from galactic to extragalactic cosmic rays occurs is not clear, but it is in the range 1017 to 1018 eV. (en) |
| rdfs:label |
الأشعة الكونية من خارج المجرة (ar) Extragalactic cosmic ray (en) |
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freebase:Extragalactic cosmic ray yago-res:Extragalactic cosmic ray wikidata:Extragalactic cosmic ray dbpedia-ar:Extragalactic cosmic ray https://global.dbpedia.org/id/4jvvh |
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