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arXiv · 0812.4465

Small-scale solar magnetic fields

A. G. de Wijn·J. O. Stenflo·S. K. Solanki·S. Tsuneta
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Abstract

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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A. G. de Wijn, J. O. Stenflo, S. K. Solanki, S. Tsuneta. 2008-12-24. Small-scale solar magnetic fields. https://doi.org/10.1007/s11214-008-9473-6

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