Upward velocities of the reconnection points and coronal magnetic field strengths in flaring regions derived from the GOES X-ray light curves
Abstract
From Yohkoh and SoHO observations, the magnetic reconnection is considered as a main energy release mechanism of the solar active phenomena. In this study, we try to reproduce GOES X-ray light curves (1-8 Å) of solar flares using a model incorporating the radiative and conductive cooling and the magnetic reconnection heating.
- Publication:
-
Solar Activity and its Magnetic Origin
- Pub Date:
- 2006
- DOI:
- 10.1017/S1743921306001669
- Bibcode:
- 2006IAUS..233..128Y