On a limitation of Zeeman polarimetry and imperfect instrumentation in representing solar magnetic fields with weaker polarization signal

Full disk vector magnetic fields are used widely for developing better understanding of large-scale structure, morphology, and patterns of the solar magnetic field. The data are also important for modeling various solar phenomena. However, observations of vector magnetic fields have one important li...

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Detalles Bibliográficos
Autores principales: Pevtsov, A.A., Liu, Y., Virtanen, I., Bertello, L., Mursula, K., Leka, K.D., Hughes, A.L.H.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: 2021
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8833097/
https://www.ncbi.nlm.nih.gov/pubmed/35154847
http://dx.doi.org/10.1051/swsc/2021003

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8833097/
https://www.ncbi.nlm.nih.gov/pubmed/35154847
http://dx.doi.org/10.1051/swsc/2021003

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