Comparison Between Hot and Cool Ejections in CME/Flare Events

Details Comparison Between Hot and Cool Ejections in CME/Flare Events Comparison Between Hot and Cool Ejections in CME/Flare Events

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh22a09n&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH22A-09

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7513 Coronal Mass Ejections, 7519 Flares

Scientific paper

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.

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