Distortion of the interplanetary magnetic field by three‐dimensional propagation of coronal mass ejections in a structured solar wind
- 1 December 1999
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 104 (A12) , 28225-28239
- https://doi.org/10.1029/1999ja900319
Abstract
No abstract availableKeywords
This publication has 33 references indexed in Scilit:
- Three‐dimensional propagation of coronal mass ejections (CMEs) in a structured solar wind flow: 1. CME launched within the streamer beltJournal of Geophysical Research, 1999
- A 2.5‐dimensional MHD parametric study of interplanetary shock interactions with the heliospheric current sheet/heliospheric plasma sheetJournal of Geophysical Research, 1998
- Influence of stream‐stream interaction on the winding angle of the IMF spiralGeophysical Research Letters, 1998
- Asymmetric propagation of flare‐generated shocks in the heliospheric equatorial planeJournal of Geophysical Research, 1998
- Streamer belt structure at solar minimaGeophysical Research Letters, 1997
- Distortion of the heliospheric plasma sheet by interplanetary shocksGeophysical Research Letters, 1996
- Geometry of interplanetary magnetic cloudsGeophysical Research Letters, 1995
- 3‐D Simulation of high‐latitude interaction regions: Comparison with Ulysses resultsGeophysical Research Letters, 1994
- Global, quasi‐steady dynamics of the distant solar wind, 1. Origin of north‐south flows in the outer heliosphereJournal of Geophysical Research, 1994
- Field line draping about fast coronal mass ejecta: A source of strong out‐of‐the‐ecliptic interplanetary magnetic fieldsGeophysical Research Letters, 1987