Classification of magnetic reconnection during two current-loop coalescence
- 1 December 1992
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 142 (2) , 399-402
- https://doi.org/10.1007/bf00151463
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- High-energy flare explosions driven by 3-dimensional X-type current loop coalescenceSolar Physics, 1991
- Elementary flare bursts explained by explosive coalescenceSolar Physics, 1991
- High-energy particle acceleration during the implosion driven by three-dimensional X-type current loop coalescence in solar flaresThe Astrophysical Journal, 1990
- Prompt particle acceleration and plasma jet formation during current loop coalescence in solar flaresThe Astrophysical Journal Supplement Series, 1990
- Coronal explosions as a signature of current loop coalescence in solar flaresSolar Physics, 1989
- Plasma jet and shock formation during current loop coalescence in solar flaresSolar Physics, 1989
- The observed characteristics of flare energy release. I - Magnetic structure at the energy release siteThe Astrophysical Journal, 1988
- A quantitative study relating observed shear in photospheric magnetic fields to repeated flaringSolar Physics, 1984
- Loop coalescence in flares and coronal X-ray brighteningThe Astrophysical Journal, 1982
- On the Origin of Solar FlaresMonthly Notices of the Royal Astronomical Society, 1960