Semiempirical Models of Solar Magnetic Structures

Details Semiempirical Models of Solar Magnetic Structures Semiempirical Models of Solar Magnetic Structures

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apjs..169..439s&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 169, Issue 2, pp. 439-457.

Astronomy and Astrophysics

Astronomy

9

Line: Profiles, Sun: Atmosphere, Sun: Chromosphere, Sun: Magnetic Fields

Scientific paper

This paper presents semiempirical models of various solar magnetic structures, extending from the photosphere to the chromosphere. The models have been derived from non-LTE inversions of high-resolution spectropolarimetric observations of four Ca II and Fe I lines. The observed targets are dark and bright components of a sunspot umbra; dark and bright components of a sunspot penumbra; a canopy between two sunspots; a facula; and a network element. These models may be employed, e.g., to compute realistic synthetic Stokes spectra of photospheric and chromospheric lines.

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