Multi-Line Spectro-Polarimetry of Filaments

Details Multi-Line Spectro-Polarimetry of Filaments Multi-Line Spectro-Polarimetry of Filaments

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..358...68b&link_type=abstract

Solar Polarization 4, ASP Conference Series, Vol. 358, Proceedings of the conference held 19-23 September, 2005, in Boulder, Col

Computer Science

Scientific paper

We present a spectro-polarimetric study of magnetic structures supporting quiescent filaments, using the combined DLSP-Phase I and ASP observations. The observations were performed using the spectral lines Fe I 6301.5 Å and 6302.5 Å at the photospheric level, and Mg I 5172.7 Å and H I 6562.8 Å (Hα) at the chromospheric level. Using non-linear, force-free extrapolation models, we reconstruct the 3D magnetic loop-geometry and compare the viability of the magnetic filament dips as the true location of the filaments, as seen in Hα.

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