Small-scale solar magnetic fields

As we resolve ever smaller structures in the solar atmosphere, it has become clear that magnetism is an important component of those small structures. Small-scale magnetism holds the key to many poorly understood facets of solar magnetism on all scales, such as the existence of a local dynamo, chromospheric heating, and flux emergence, to name a few. Here, we review our knowledge of small-scale photospheric fields, with particular emphasis on quiet-sun field, and discuss the implications of several results obtained recently using new instruments, as well as future prospects in this field of research.

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Copyright Springer Science+Business Media B.V. 2008.
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Author de Wijn, Alfred
Stenflo, J.
Solanki, S.
Tsuneta, S.
Publisher UCAR/NCAR - Library
Publication Date 2009-04-01T00:00:00
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Topic Category geoscientificInformation
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Metadata Date 2023-08-18T18:45:06.512414
Metadata Record Identifier edu.ucar.opensky::articles:15441
Metadata Language eng; USA
Suggested Citation de Wijn, Alfred, Stenflo, J., Solanki, S., Tsuneta, S.. (2009). Small-scale solar magnetic fields. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d7dz09bq. Accessed 19 June 2025.

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