Chromospheric evaporation in sympathetic coronal bright points
Q. M. ZhangKey Lab of Modern Astronomy and Astrophysics, Ministry of Education, PR ChinaHaisheng JiKey Laboratory for Dark Matter and Space Science, Purple Mountain Observatory, CAS, 210008 Nanjing, PR China
2013en
ABI
Abstract
Context. Chromospheric evaporation is a key process in solar flares that has been extensively investigated using spectroscopic observations. However, direct soft X-ray (SXR) imaging of the process is rare, especially in remote brightenings associated with the primary flares that have recently attracted a great deal of attention.
Identifiers
Citations and references
Cited by 20 references