Solar chromospheric flares: energy release, transport and radiation
arXiv:1207.0384
Abstract
This paper presents an overview of some recent observational and theoretical results on solar flares, with an emphasis on flare impulsive-phase chromospheric properties, including: electron diagnostics, optical and UV emission, and discoveries made by the Hinode mission, especially in the EUV. A brief perspective on future observations and theoretical requirements is also given
arXiv comment11 pages, 2 Figures
References in corpus (4)
- Radiative Hydrodynamic Models of the Optical and Ultraviolet Emission from Solar Flares
- RHESSI and SOHO/CDS Observations of Explosive Chromospheric Evaporation
- Difference between Spatial Distributions of the H-alpha Kernels and Hard X-Ray Sources in a Solar Flare
- Transition Region Emission and Energy Input to Thermal Plasma During the Impulsive Phase of Solar Flares