Photospheric magnetic field and chromospheric emission
Astrophysics
2007-05-23 v1
Abstract
We present a statistical analysis of network and internetwork properties in the photosphere and the chromosphere. For the first time we simultaneously observed (a) the four Stokes parameters of the photospheric iron line pair at 630.2 nm and (b) the intensity profile of the Ca II H line at 396.8 nm. The vector magnetic field was inferred from the inversion of the iron lines. We aim at an understanding of the coupling between photospheric magnetic field and chromospheric emission.
Cite
@article{arxiv.astro-ph/0701681,
title = {Photospheric magnetic field and chromospheric emission},
author = {R. Rezaei and R. Schlichenmaier and C. Beck and W. Schmidt},
journal= {arXiv preprint arXiv:astro-ph/0701681},
year = {2007}
}
Comments
4 pages, appeared in "Modern Solar Facilities: Advanced Solar Sciences", Eds. F. Kneer, K.G. Puschmann, A.D.Wittmann, Sep. 2006