Why Do Temperature and Velocity Have Different Relationships in the Solar Wind and in Interplanetary Coronal Mass Ejections?
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-009-9338-5.pdf
Reference38 articles.
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2. Cargill, P.J., Schmidt, J.M.: 2002, Modelling interplanetary CMEs using magnetohydrodynamic simulations. Ann. Geophys. 20, 879 – 890.
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4. Chen, J.: 1996, Theory of prominence eruption and propagation: Interplanetary consequences. J. Geophys. Res. 101, 27499 – 27520. doi: 10.1029/96JA02644 .
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