Transverse oscillations and an energy source in a strongly magnetized sunspot
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 temperature. Using the 1.6 m Goode Solar Telescope, we report a detection of ubiquitous and persistent transverse waves in umbral
Yuan, Ding et al.
Fecha de publicación:
7
2023