PLASMA NEAR THE HELIOSHEATH: OBSERVATIONS AND MODELING
Author(s)
Borovikov, Sergey N.; Pogorelov, Nikolai V.; Burlaga, L. F.; Richardson, John D.
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Sound numerical modeling is capable of providing important predictive information about the solar wind interaction with the local interstellar medium. The results of our three-dimensional simulation show a good agreement with Voyager observations from 2007 to 2010. We analyze the termination shock properties at the Voyager crossing points and juxtapose them with the observed data. The heliospheric current sheet structure in the inner heliosheath is examined.
Date issued
2011-01Department
MIT Kavli Institute for Astrophysics and Space ResearchJournal
Astrophysical Journal. Letters
Publisher
IOP Publishing
Citation
Borovikov, Sergey N., Nikolai V. Pogorelov, Leonard F. Burlaga, and John D. Richardson. “PLASMA NEAR THE HELIOSHEATH: OBSERVATIONS AND MODELING.” The Astrophysical Journal 728, no. 1 (January 24, 2011): L21. © 2011 The American Astronomical Society
Version: Author's final manuscript
ISSN
2041-8205
2041-8213