Three-dimensional MHD simulation of interplanetary magnetic field changes at 1 AU as a consequence of simulated solar flares
A fully three-dimensional (3D), time-dependent, MHD interplanetary global model (3D IGM) has been used, for the first time, to study the relationship between different forms of solar activity and transient variations of the north-south component, <i>B<sub>z</sub></i>, of...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
1996-04-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/14/383/1996/angeo-14-383-1996.pdf |