Thursday, March 22, 2012

1203.4577 (J. de la Cruz Rodríguez et al.)

Chromospheric magnetic fields. Observations, simulations and their interpretation    [PDF]

J. de la Cruz Rodríguez, H. Socas-Navarro, M. Carlsson, J. Leenaarts
The magnetic field of the quiet-Sun chromosphere remains a mystery for solar physicists. The reduced number of chromospheric lines are intrinsically hard to model and only a few of them are magnetically sensitive. In this work, we use a 3D numerical simulation of the outer layers of the solar atmosphere, to asses the reliability of non-LTE inversions, in this case applied to the Ca II 8542 \AA\ line. We show that NLTE inversions provide realistic estimates of physical quantities from synthetic observations.
View original: http://arxiv.org/abs/1203.4577

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