Magnetic field inversions from Stokes profiles generated by MHD simulations

Bibcode
2007MmSAI..78..166K
Khomenko, E.; Collados, M.
Bibliographical reference

Memorie della Società Astronomica Italiana, v.78, p.166 (2006)

Advertised on:
0
2007
Number of authors
2
IAC number of authors
2
Citations
4
Refereed citations
3
Description
We report tests of inversion methods applied to complex Stokes spectra generated by realistic MHD simulations. The average magnetic field strength of the simulations used is of 30 and 140 G, which we believe is representative of quiet solar regions. The behaviour of the Fe I at 1.56 mu m and 630 nm lines is analyzed. The tests have been done with the original resolution of simulations (20 km) and also with resolution of 0.6'' and 1.4'' (after having conveniently degraded the images).
Type
Non-refereed
Magnetic fields

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