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...

Бүрэн тодорхойлолт

Номзүйн дэлгэрэнгүй
Үндсэн зохиолчид: James A. Klimchuk, Kalman J. Knizhnik, Vadim M. Uritsky
Формат: Өгүүллэг
Хэл сонгох:English
Хэвлэсэн: IOP Publishing 2022-01-01
Цуврал:The Astrophysical Journal
Нөхцлүүд:
Онлайн хандалт:https://doi.org/10.3847/1538-4357/ac9f41