Search for GeV neutrino emission during intense gamma-ray solar flares with the IceCube Neutrino Observatory
Solar flares convert magnetic energy into thermal and non-thermal plasma energy, the latter implying particle acceleration of charged particles such as protons. Protons are injected out of the coronal acceleration region and can interact with dense plasma in the lower solar atmosphere, producing...
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| Μορφή: | Άρθρο |
| Γλώσσα: | English |
| Έκδοση: |
American Physical Society (APS)
2022
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| Διαθέσιμο Online: | https://hdl.handle.net/1721.1/142018 |