The inference of the 3-D structure of solar vector magnetic fields and thermodynamics from Stokes profiles.

Details The inference of the 3-D structure of solar vector magnetic fields and thermodynamics from Stokes profiles. The inference of the 3-D structure of solar vector magnetic fields and thermodynamics from Stokes profiles.

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acasn..37..201q&link_type=abstract

Acta Astron. Sin., Vol. 37, No. 2, p. 201 - 211

Astronomy and Astrophysics

Astronomy

Solar Atmosphere: Radiative Transfer, Solar Magnetic Fields: Structure

Scientific paper

A new method to infer the three-dimensional structure of vector magnetic fields and thermodynamics from Stokes profile analysis is presented. The method consists of three coupled operations. These form an executive unit. Applying this unit to every depth devided from the surface to the bottom of the photosphere, and then the same procedure to the Stokes profiles of every scanning point, the structure of the scanning region can be obtained. Detailed description of these 3-D operations is given and a flow diagram is plotted.

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