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Distortions of CMEs and IMF in the structured solar wind
- 1.0124564 - ASU-R 20000018 RIV NL eng C - Conference Paper (international conference)
Odstrčil, Dušan - Pizzo, V. J.
Distortions of CMEs and IMF in the structured solar wind.
Magnetic fields and solar processes. Noordwijk: ESA Publications Division, 1999 - (Wilson, A.), s. 987-990. ISBN 92-9092-792-5.
[European meeting on solar physics /9./. Florence (IT), 12.09.1999-18.09.1999]
R&D Projects: GA AV ČR IAA3003707
Grant - others:-(US) NAGW-4616
Institutional research plan: CEZ:AV0Z1003909
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
A 3-D numerical magnetohydrodynamic model is used to investigate propagation of coronal mass ejections (CME) in the structured solar wind. Numerical results show that the motion and appearance of a CME are affected by its interaction with the velocity and density structure of the background solar wind.
Permanent Link: http://hdl.handle.net/11104/0022823
Number of the records: 1