Yuan, Ding; Fu, Libo; Cao, Wenda; Kuźma, Błażej; Geeraerts, Michaël; Trelles Arjona, Juan C.; Murawski, Kris; Van Doorsselaere, Tom; Srivastava, Abhishek K.; Miao, Yuhu; Feng, Song; Feng, Xueshang
(Nature Research, 2023-05-25)
The solar corona is two to three orders of magnitude hotter than the underlying photosphere, and the energy loss of coronal plasma is extremely strong, requiring a heating flux of over 1,000 W m −2 to maintain its high ...