An Explainable Deep-learning Model of Proton Auroras on Mars
Proton auroras are widely observed on the dayside of Mars, identified as a significant intensity enhancement in the hydrogen Ly α (121.6 nm) emission at altitudes of ∼110 and 150 km. Solar wind protons penetrating as energetic neutral atoms into Mars’ thermosphere are thought to be primarily respons...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
IOP Publishing
2024-01-01
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| Σειρά: | The Planetary Science Journal |
| Θέματα: | |
| Διαθέσιμο Online: | https://doi.org/10.3847/PSJ/ad45ff |
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