Magnetohydrodynamic modeling of prominence formation within a helmet streamer
- 1 November 2001
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 106 (A11), 25165-25175
- https://doi.org/10.1029/2000ja004020
Abstract
No abstract availableThis publication has 45 references indexed in Scilit:
- A Twisted Flux Rope Model for Coronal Mass Ejections and Two-Ribbon FlaresThe Astrophysical Journal, 2000
- Three-dimensional Solutions of Magnetohydrodynamic Equationsfor Prominence Magnetic Support: Twisted Magnetic Flux RopeThe Astrophysical Journal, 1999
- The Dynamic Formation of Prominence CondensationsThe Astrophysical Journal, 1999
- A Model for Solar Coronal Mass EjectionsThe Astrophysical Journal, 1999
- The Magnetic Topology of Solar EruptionsThe Astrophysical Journal, 1998
- Theory of prominence eruption and propagation: Interplanetary consequencesJournal of Geophysical Research, 1996
- The magnetic field of solar prominencesThe Astrophysical Journal, 1994
- A model for the formation of solar prominencesThe Astrophysical Journal, 1991
- Radiation loss rates in Lyman-alpha for solar conditionsThe Astrophysical Journal, 1986
- On some properties of force-free magnetic fields in infinite regions of spaceThe Astrophysical Journal, 1984