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Paper: INVERS10: A New Code for Magnetic Doppler Imaging
Volume: 154, Cool Stars, Stellar Systems and the Sun: Tenth Cambridge Workshop
Page: 2029
Authors: Piskunov, N.
Abstract: We present a new Magnetic Doppler Imaging computer code designed to simultaneously reconstruct both the 3D structure of magnetic fields and the temperature structure of active regions on the surfaces of late-type stars. We show results from numerical experiments and demonstrate that the full set Stokes parameters is needed for proper reconstruction of the magnetic field vector.
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