Spectropolarimetric Investigations of the Deep Photospheric Layers of Solar Magnetic Structures

Details Spectropolarimetric Investigations of the Deep Photospheric Layers of Solar Magnetic Structures Spectropolarimetric Investigations of the Deep Photospheric Layers of Solar Magnetic Structures

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..405..233o&link_type=abstract

Solar Polarization 5: In Honor of Jan Stenflo ASP Conference Series, Vol. 405, proceedings of the conference held 17-21 Septembe

Astronomy and Astrophysics

Astronomy

Scientific paper

Solar surface magnetism manifests itself in a variety of structures with sizes often comparable or even below our spatial resolution capabilities. Nevertheless, sub-resolution information about the intrinsic atmospheric structure can be obtained via indirect techniques. We use state-of-the-art spectropolarimetric observations in carefully selected photospheric lines which include C~I~(5380.3~Å) as well as strong lines of Fe~I, Ti~I covering also the deep layers of the photosphere and obtain ratios of their Stokes V amplitudes. From there we deduce that the temperature within magnetic features is higher at locations of smaller magnetic flux.

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