Articles | Volume 22, issue 12
https://doi.org/10.5194/angeo-22-4397-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-22-4397-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
22 Dec 2004
Non-radial solar wind flows induced by the motion of interplanetary coronal mass ejections
M. Owens
now at: Center for Space Physics Boston University, Boston MA 02215,
Space and Atmospheric Physics, The Blackett Laboratory Imperial College, London SW7 2BW, UK
P. Cargill
Space and Atmospheric Physics, The Blackett Laboratory Imperial College, London SW7 2BW, UK
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Cited
42 citations as recorded by crossref.
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- MAGNETIC FIELD-LINE LENGTHS IN INTERPLANETARY CORONAL MASS EJECTIONS INFERRED FROM ENERGETIC ELECTRON EVENTS S. Kahler et al. 10.1088/0004-637X/736/2/106
- Beyond Basic Drag in Interplanetary CME Modeling: Effects of Solar Wind Pileup and High‐Speed Streams C. Kay et al. 10.1029/2022SW003165
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- Thermospheric nitric oxide response to shock‐led storms D. Knipp et al. 10.1002/2016SW001567
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- LEARNING FROM THE OUTER HELIOSPHERE: INTERPLANETARY CORONAL MASS EJECTION SHEATH FLOWS AND THE EJECTA ORIENTATION IN THE LOWER CORONA R. Evans et al. 10.1088/0004-637X/728/1/41
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Latest update: 04 Nov 2025
