Spectral signature of uncombed penumbral magnetic fields. Comment

Details Spectral signature of uncombed penumbral magnetic fields. Comment Spectral signature of uncombed penumbral magnetic fields. Comment

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...369..643s&link_type=abstract

Astronomy and Astrophysics, v.369, p.643 (2001)

Astronomy and Astrophysics

Astrophysics

11

Sun: Magnetic Fields, Sunspots

Scientific paper

The conservation of magnetic flux demands a magnetic field fine structure as small as 15 km to explain the net circular polarization observed in penumbrae (Sánchez Almeida \cite{san98a}). A recent work by Martínez Pillet (\cite{mar00}) claims that modeling penumbrae as a collection of fluxtubes 100 km wide suffices. We identify several shortcomings of such modeling so that it is presently unclear whether it really contradicts the former conclusion.

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