AbstractRecent observations and theoretical developments have re-awakened interest in finding out what happens at the boundary between closed and open magnetic field regions in the solar corona, i.e., between coronal loops and coronal holes. We model the boundary region between closed and open magnetic field regions, i.e., coronal loops and coronal holes. Both linear and nonlinear properties are explored. An acceleration of plasma along the coronal hole magnetic field direction is observed. Published by Elsevier Ltd on behalf of COSPAR.
Modelling the coronal hole-coronal loop boundary as a compressible current-vortex sheet
Advances in Space Research ; 32 , 6 ; 1125-1130
2003-01-31
6 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Modelling the coronal hole-coronal loop boundary as a compressible current-vortex sheet
Online Contents | 2003
|Modelling the Coronal Hole-Coronal Loop Boundary as a Compressible Current-Vortex Sheet
British Library Conference Proceedings | 2003
|Morphology of Coronal Loop Interactions
British Library Online Contents | 1992
|RESONANTLY DAMPED CORONAL LOOP OSCILLATIONS
British Library Conference Proceedings | 2005
|DYNAMICS OF CORONAL LOOP OSCILLATIONS
British Library Conference Proceedings | 2005
|