A Magnetic Map of a Solar Filament

Bibcode
2007ASPC..368..347M
Merenda, L.; Trujilo-Bueno, J.; Collados, M.
Referencia bibliográfica

The Physics of Chromospheric Plasmas ASP Conference Series, Vol. 368, Proceedings of the conference held 9-13 October, 2006 at the University of Coimbra in Coimbra, Portugal. Edited by P. Heinzel, I. Dorotovič, and R. J. Rutten. San Francisco: Astronomical Society of the Pacific, 2007., p.347

Fecha de publicación:
5
2007
Número de autores
3
Número de autores del IAC
0
Número de citas
10
Número de citas referidas
8
Descripción
One of the most useful diagnostic tools for the detection of inclined magnetic fields in solar chromospheric and coronal structures is that based on the fact that the Hanle effect in forward scattering at the solar disk center creates linear polarization in some spectral lines, such as those of the He I 10830 Å multiplet. Here we show the preliminary results of an ongoing investigation on the magnetic field of a solar filament, based on the inversion of spectropolarimetric observations obtained with the Tenerife Infrared Polarimeter.
Tipo
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