Mapping solar magnetic fields from the photosphere to the base of the corona.
Journal
Science advances
ISSN: 2375-2548
Titre abrégé: Sci Adv
Pays: United States
ID NLM: 101653440
Informations de publication
Date de publication:
Feb 2021
Feb 2021
Historique:
received:
17
09
2020
accepted:
08
01
2021
entrez:
20
2
2021
pubmed:
21
2
2021
medline:
21
2
2021
Statut:
epublish
Résumé
Routine ultraviolet imaging of the Sun's upper atmosphere shows the spectacular manifestation of solar activity; yet, we remain blind to its main driver, the magnetic field. Here, we report unprecedented spectropolarimetric observations of an active region plage and its surrounding enhanced network, showing circular polarization in ultraviolet (Mg ii
Identifiants
pubmed: 33608278
pii: 7/8/eabe8406
doi: 10.1126/sciadv.abe8406
pmc: PMC7895431
pii:
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM
Informations de copyright
Copyright © 2021 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC).
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