Acceleration of Energetic Ions in Corotating Interaction Region near 1.5 au: Evidence from MAVEN
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/ab2b43/pdf
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1. Differences between CME-driven storms and CIR-driven storms
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5. The suprathermal seed population for corotating interaction region ions at 1 AU deduced from composition and spectra of H+, He++, and He+observed on Wind
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