Structure of solar magnetic fluxtubes from the inversion of Stokes spectra at disk center

Details Structure of solar magnetic fluxtubes from the inversion of Stokes spectra at disk center Structure of solar magnetic fluxtubes from the inversion of Stokes spectra at disk center

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...233..583k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 2, July 1990, p. 583-597.

Astronomy and Astrophysics

Astrophysics

70

Solar Magnetic Field, Solar Spectra, Stokes Law Of Radiation, Two Dimensional Models, Fourier Transformation, Line Spectra, Solar Atmosphere

Scientific paper

The paper presents an inversion procedure that derives the temperature stratification, the turbulent velocity, and the magnetic field strength of the photospheric layers of small-scale magnetic fields from observed Stokes V spectra and the continuum intensity. The inversion is based on the determination of a small number of model flux parameters by a nonlinear least squares fitting algorithm. The minimization of the sum of the squared differences between observed and synthetic observables makes it possible to determine the temperature stratification and the magnetic field strength.

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