Quantifying the Difference Between the Flux-Tube Expansion Factor at the Source Surface and at the Alfvén Surface Using a Global MHD Model for the Solar Wind-Reference-Cited by-同舟云学术

Quantifying the Difference Between the Flux-Tube Expansion Factor at the Source Surface and at the Alfvén Surface Using a Global MHD Model for the Solar Wind

Published:2015-07-29 Issue:8 Volume:290 Page:2245-2263
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Cohen O.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-015-0739-3.pdf

Reference34 articles.

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5. DeForest, C.E., Howard, T.A., McComas, D.J.: 2014, Inbound waves in the solar corona: a direct indicator of Alfvén surface location. Astrophys. J. 787, 124. DOI . ADS .

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