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Likely Common Coronal Source of Solar Wind and 3He-Enriched Energetic Particles: Uncoupled Transport from the Low Corona to 0.2 Au

D. G. Mitchell,M. E. Hill,D. J. Mccomas,C. M. S. Cohen,N. A. Schwadron,P. S. Mostafavi,W. H. Matthaeus,N. E. Raouafi,S. T. Al-Nussirat,D. E. Larson,A. Rahmati,J. C. Kasper,P. L. Whittlesey,R. Livi,S. D. Bale,M. Pulupa,J. Giacalone,R. L. Mcnutt,E. R. Christian,M. E. Wiedenbeck,T. Sharma

ASTROPHYSICAL JOURNAL（2024）

Cited 2|Views40
Key words
Solar energetic particles,Solar physics,Solar abundances,Solar wind,Solar activity
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