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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Detalles Bibliográficos
Autores principales: 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.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: 2019
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7370956/
https://www.ncbi.nlm.nih.gov/pubmed/32690977
http://dx.doi.org/10.3847/1538-4357/ab23f1

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7370956/
https://www.ncbi.nlm.nih.gov/pubmed/32690977
http://dx.doi.org/10.3847/1538-4357/ab23f1

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