Consequences of Treating the Solar Magnetic Field as a Dipole on the Global Structure of the Heliosphere and Heliosheath
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/860/i=2/a=171/pdf
Reference44 articles.
1. Kinetic vs. multi-fluid models of H atoms in the heliospheric interface: a comparison
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3. Model of the solar wind interaction with the local interstellar medium: Numerical solution of self-consistent problem
4. PLASMA NEAR THE HELIOSHEATH: OBSERVATIONS AND MODELING
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