Dynamics of Large‐Scale Solar‐Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance
Author:
Affiliation:
1. Space Research Institute (IKI) Russian Academy of Sciences Moscow Russia
2. Skobeltsyn Institute of Nuclear Physics Lomonosov Moscow State University Moscow Russia
3. P.N. Lebedev Physical Institute Russian Academy of Sciences Moscow Russia
Funder
Russian Science Foundation
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JA027878
Reference45 articles.
1. Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU?
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