Hot plasma and non-thermal particles in small flares
Abstract
I will discuss how high resolution current (e.g., Hinode, SDO, IRIS, SolO), and future (e.g., MUSE and EUVST), UV, EUV and X-ray observations of the solar atmosphere, and in particular spectroscopy, help us advance our understanding of the coronal plasma properties in small (nano- to micro-) flares.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2022
- Bibcode:
- 2022AGUFMSH22B..01T