ON THE NATURE OF RECONNECTION AT A SOLAR CORONAL NULL POINT ABOVE A SEPARATRIX DOME
Authors:
- D. I. PontinDPD. I. Pontin
- E. R. PriestEPE. R. Priest
- K. GalsgaardKGK. Galsgaard
- 26 August 2013
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 774 (2)
Abstract
No abstract availableAll Related Versions
This publication has 41 references indexed in Scilit:
- Magnetohydrodynamics dynamical relaxation of coronal magnetic fieldsAstronomy & Astrophysics, 2012
- INTERCHANGE RECONNECTION AND CORONAL HOLE DYNAMICSThe Astrophysical Journal, 2010
- Structure and Dynamics of the Sun’s Open Magnetic FieldThe Astrophysical Journal, 2007
- On the Relationship between Coronal Magnetic Null Points and Solar Eruptive EventsThe Astrophysical Journal, 2007
- Separator reconnection at Earth's dayside magnetopause under generic northward interplanetary magnetic field conditionsJournal of Geophysical Research, 2007
- Slip-Running Reconnection in Quasi-Separatrix LayersSolar Physics, 2006
- Numerical experiments on wave propagation towards a 3D null point due to rotational motionsJournal of Geophysical Research, 2003
- Reducing heliospheric magnetic flux from coronal mass ejections without disconnectionJournal of Geophysical Research, 2002
- Magnetic Collapse in Incompressible Plasma FlowsJournal of the Physical Society of Japan, 1997
- Exact Solutions for Steady State, Spine, and Fan Magnetic ReconnectionThe Astrophysical Journal, 1996