Heating and activity of the solar corona: 2. Kink instability in a flux tube
- 1 January 1997
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 102 (A1) , 219-230
- https://doi.org/10.1029/96ja01462
Abstract
No abstract availableKeywords
This publication has 16 references indexed in Scilit:
- Heating and activity of the solar corona: 1. Boundary shearing of an initially homogeneous magnetic fieldJournal of Geophysical Research, 1996
- Scaling of heating rates in solar coronal loopsNature, 1995
- Nonlinear MagnetohydrodynamicsPublished by Cambridge University Press (CUP) ,1993
- Dynamical evolution of twisted magnetic flux tubes. I - Equilibrium and linear stabilityThe Astrophysical Journal, 1990
- Nonlinear development of the kink instability in coronal flux tubesThe Astrophysical Journal, 1990
- The linear stability of line-tied coronal magnetic fieldsThe Astrophysical Journal, 1990
- Non-linear saturation of the internal kink modeNuclear Fusion, 1980
- Magnetic instability of coronal arcades as the origin of two-ribbon flaresSolar Physics, 1980
- Kink instability of solar coronal loops as the cause of solar flaresSolar Physics, 1979
- The stability of force-free magnetic fields with cylindrical symmetry in the context of solar flaresSolar Physics, 1968