Spectropolarimetry in the chromospheric He I 1083.0 nm multiplet

Details Spectropolarimetry in the chromospheric He I 1083.0 nm multiplet Spectropolarimetry in the chromospheric He I 1083.0 nm multiplet

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007waas.work...43s&link_type=abstract

"1st Workshop of Astronomy and Astrophysics for Students" held in Naples (ITALY) on April 19-20, 2006. Published by INFN-Naples,

Astronomy and Astrophysics

Astrophysics

Scientific paper

Spectropolarimetry in the He I 1083.0 nm multiplet has a great potential to obtain information on the magnetic field in the solar upper chromosphere. We apply an inversion technique to infrared spectropolarimetric observations, to retrieve the full magnetic vector and the line-of sight velocity. The observations, obtained with the Tenerife Infrared Polarimeter (TIP) II at the German Vacuum Tower Telescope (VTT), provide maps in the Stokes parameters I, Q, U and V.

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