Theory of magnetic connectivity in the solar corona
Top Cited Papers
- 6 August 2002
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 107 (A8), SSH 3-1-SSH 3-13
- https://doi.org/10.1029/2001ja000278
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- Thin current sheets and magnetotail dynamicsJournal of Geophysical Research, 1999
- Quasi‐Separatrix Layers in a Reduced Magnetohydrodynamic Model of a Coronal LoopThe Astrophysical Journal, 1999
- Formation of current layers in three‐dimensional, inhomogeneous coronal magnetic fields by photospheric motionsJournal of Geophysical Research, 1997
- Three‐dimensional magnetic reconnection without null points: 2. Application to twisted flux tubesJournal of Geophysical Research, 1996
- Three‐dimensional magnetic reconnection without null points: 1. Basic theory of magnetic flippingJournal of Geophysical Research, 1995
- The form of ideal current layers in line-tied magnetic fieldsThe Astrophysical Journal, 1994
- Magnetic nulls and topology in a class of solar flare modelsSolar Physics, 1993
- Photospheric vortex flows as a cause for two-ribbon flares: A topological modelSolar Physics, 1988
- Spontaneous formation of electric current sheets and the origin of solar flaresThe Astrophysical Journal, 1988
- Flux linkages of bipolar sunspot groups: A computer studySolar Physics, 1980