Comparison Between Hot and Cool Ejections in CME/Flare Events
Abstract
Comparison between hot and cool ejections in CME/flare events Nariaki Nitta (LMSAL) , Sachiko Akiyama (GUAS) We have shown that high-temperature ejections during the impulsive phase of flares as seen with Yohkoh/SXT are correlated with coronal mass ejections (CMEs) as seen by SOHO/LASCO. Since then we have collected a number of examples of ejections observed with TRACE. In this presentation, we compare ejections in soft X-rays with those in H-alpha and EUV, and study the sequence of processes (reconnection, mass motion, heating, etc.) involved in CMEs so that we can put more constraints on the models.
- Publication:
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AGU Spring Meeting Abstracts
- Pub Date:
- May 2001
- Bibcode:
- 2001AGUSM..SH22A09N
- Keywords:
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- 7500 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7513 Coronal mass ejections;
- 7519 Flares