Abstract |
In association with strong solar flares, we sometimes observe enhancements of visible continuum
radiation, which is known as a "white-light flare (WLF)". As most white-light (WL) events show close
correlations in time and location with hard X-rays and/or radio emission, there is some consensus that
WL emission originates from accelerated particles, especially non-thermal electrons. However, the
generation mechanism of WLF has not yet been elucidated.
In this talk, we report the statistical properties of WLFs, and discuss the possibility that other candidates
(accelerated protons etc.) may produce the WLFs. We will then discuss the dynamics of high-energy
phenomena in the source regions of solar flares, especially in the low solar atmosphere. |