Bibcode
DOI
Socas-Navarro, H.
Referencia bibliográfica
The Astrophysical Journal Supplement Series, Volume 169, Issue 2, pp. 439-457.
Advertised on:
4
2007
Número de citas
31
Número de citas referidas
29
Descripción
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.