Abstract
Observations of the reconnection process between two magnetic fluxes are presented. The lower reconnecting flux seemed to be a rising post-flare loop system, the upper one a giant magnetic loop of the active region. The interaction produced a giant arch visible in the H α line center.
Original language | English (US) |
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Pages (from-to) | 199-202 |
Number of pages | 4 |
Journal | Solar Physics |
Volume | 154 |
Issue number | 1 |
DOIs | |
State | Published - Sep 1994 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science