On the fine structure of magnetic fields in sunspot penumbrae

Details On the fine structure of magnetic fields in sunspot penumbrae On the fine structure of magnetic fields in sunspot penumbrae

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...452.1089t&link_type=abstract

Astronomy and Astrophysics, Volume 452, Issue 3, June IV 2006, pp.1089-1090

Astronomy and Astrophysics

Astrophysics

6

Sunspots, Sun: Magnetic Fields

Scientific paper

Recent observations have revealed the interlocking-comb structure of the magnetic field in the outer penumbra of a sunspot. We have argued that this structure owes its origin in part to downward pumping of magnetic flux by vigorous granular convection in the region surrounding the spot. Here we stress the difference between the inner and outer penumbra, and correct some misleading assertions in a recent paper by Spruit & Scharmer.

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