DO COROTATING INTERACTION REGION ASSOCIATED SHOCKS SURVIVE WHEN THEY PROPAGATE INTO THE HELIOSHEATH?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference26 articles.
1. Interaction of interplanetary shocks with the heliospheric termination shock: Two-dimensional magnetohydrodynamic model
2. Possible crossing of the termination shock in the solar wind by the Voyager 1 spacecraft
3. SOLAR ROTATION EFFECTS ON THE HELIOSHEATH FLOW NEAR SOLAR MINIMA
4. Corotating pressure waves without fast streams in the solar wind
Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. MSWIM2D: Two-dimensional Outer Heliosphere Solar Wind Modeling;The Astrophysical Journal Supplement Series;2022-06-01
2. Interstellar Neutrals, Pickup Ions, and Energetic Neutral Atoms Throughout the Heliosphere: Present Theory and Modeling Overview;Space Science Reviews;2022-04
3. Inner Heliosheath Shocks and Their Effect on Energetic Neutral Atom Observations by IBEX;The Astrophysical Journal;2019-06-12
4. Corotating interaction regions and the 27 day variation of galactic cosmic rays intensity at 1 AU during the cycle 23/24 solar minimum;Journal of Geophysical Research: Space Physics;2014-04
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