Element Abundances: A New Diagnostic for the Solar Wind

We examine the different element abundances exhibited by the closed loop solar corona and the slow speed solar wind. Both are subject to the first ionization potential (FIP) effect, the enhancement in coronal abundance of elements with FIP below 10 eV (e.g., Mg, Si, Fe) with respect to high-FIP elem...

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Foilsithe in:Astrophys J
Main Authors: Laming, J. Martin, Vourlidas, Angelos, Korendyke, Clarence, Chua, Damien, Cranmer, Steven R., Ko, Yuan-Kuen, Kuroda, Natsuha, Provornikova, Elena, Raymond, John C., Raouafi, Nour-Eddine, Strachan, Leonard, Tun-Beltran, Samuel, Weberg, Micah, Wood, Brian E.
Formáid: Artigo
Teanga:Inglês
Foilsithe: 2019
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Article
Rochtain Ar Líne:https://ncbi.nlm.nih.gov/pmc/articles/PMC7370956/
https://ncbi.nlm.nih.gov/pubmed/32690977
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-4357/ab23f1
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