Formation of current layers in three‐dimensional, inhomogeneous coronal magnetic fields by photospheric motions
- 1 October 1997
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 102 (A10), 22285-22293
- https://doi.org/10.1029/97ja01674
Abstract
No abstract availableThis publication has 7 references indexed in Scilit:
- 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 flipping: Reconnection in three dimensions without null pointsJournal of Geophysical Research, 1992
- Electric currents in the solar corona and the existence of magnetostatic equilibriumThe Astrophysical Journal, 1985
- Magnetic neutral sheets in evolving fields. I - General theory. II - Formation of the solar coronaThe Astrophysical Journal, 1983
- Topological Dissipation and the Small-Scale Fields in Turbulent GasesThe Astrophysical Journal, 1972