Simulated XRT and EIS Observations of Magnetic Reconnection in Coronal Mass Ejection and X-Ray Arcade
Abstract
We perform a numerical simulation of a coronal mass ejection and an associated X-ray arcade. Based on the numerical results, we synthesize theoretical images taken with XRT and EIS aboard SolarB, and discuss how reconnection inflow and slow shocks would be observed with XRT and EIS. The mechanism of dimming is also discussed.
- Publication:
-
The Solar-B Mission and the Forefront of Solar Physics
- Pub Date:
- December 2004
- Bibcode:
- 2004ASPC..325..373S