Comparing Values of the Relative Magnetic Helicity in Finite Volumes
- 15 March 2012
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 278 (2) , 347-366
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Dynamical evolution of a magnetic cloud from the Sun to 5.4 AUAstronomy & Astrophysics, 2011
- A MODEL FOR MAGNETICALLY COUPLED SYMPATHETIC ERUPTIONSThe Astrophysical Journal Letters, 2011
- Testing magnetofrictional extrapolation with the Titov-Démoulin model of solar active regionsAstronomy & Astrophysics, 2010
- Nonlinear Force‐free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass EjectionThe Astrophysical Journal, 2008
- Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar CoronaThe Astrophysical Journal, 2007
- Torus InstabilityPhysical Review Letters, 2006
- Confined and Ejective Eruptions of Kink-unstable Flux RopesThe Astrophysical Journal, 2005
- A Three-dimensional Flux Rope Model for Coronal Mass Ejections Based on a Loss of EquilibriumThe Astrophysical Journal, 2003
- Magnetic Helicity Generation by Solar Differential RotationThe Astrophysical Journal, 2000
- The topological properties of magnetic helicityJournal of Fluid Mechanics, 1984