Space Science Reviews

, 144:275

Small-Scale Solar Magnetic Fields

Authors

    • University Corporation for Atmospheric Research
  • J. O. Stenflo
    • Institute of AstronomyETH Zurich
  • S. K. Solanki
    • Max-Planck-Institut für Sonnensystemforschung
  • S. Tsuneta
    • National Astronomical Observatory
Open AccessArticle

DOI: 10.1007/s11214-008-9473-6

Cite this article as:
de Wijn, A.G., Stenflo, J.O., Solanki, S.K. et al. Space Sci Rev (2009) 144: 275. doi:10.1007/s11214-008-9473-6

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.

Keywords

Sun Photosphere Magnetism Small scale

Copyright information

© Springer Science+Business Media B.V. 2008