Observational Signatures of Coronal Heating in Magnetohydrodynamic Simulations without Radiation or a Lower Atmosphere
It is extremely difficult to simulate the details of coronal heating and also make meaningful predictions of the emitted radiation. Thus, testing realistic models with observations is a major challenge. Observational signatures of coronal heating depend crucially on radiation, thermal conduction, an...
Үндсэн зохиолчид: | , , |
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Формат: | Өгүүллэг |
Хэл сонгох: | English |
Хэвлэсэн: |
IOP Publishing
2022-01-01
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Цуврал: | The Astrophysical Journal |
Нөхцлүүд: | |
Онлайн хандалт: | https://doi.org/10.3847/1538-4357/ac9f41 |