Issue |
A&A
Volume 414, Number 3, February II 2004
|
|
---|---|---|
Page(s) | 1109 - 1120 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20031643 | |
Published online | 27 January 2004 |
Retrieval of the full magnetic vector with the He I multiplet at 1083 nm
Maps of an emerging flux region
Max-Planck-Institut für Aeronomie, Max-Planck-Str. 2, Katlenburg-Lindau, Germany
Corresponding author: A. Lagg, lagg@linmpi.mpg.de
Received:
9
July
2003
Accepted:
21
October
2003
A technique is presented to invert Stokes profiles of the He I 1083 nm multiplet lines in order to obtain the full magnetic vector and the line-of-sight velocity. The technique makes use of spectropolarimetry connected with the Zeeman effect supplemented by a simple Hanle effect based diagnostic when appropriate. It takes into account effects like line saturation, magnetooptical effects, etc. and is coupled with a genetic algorithm, which ensures that the global minimum in a goodness of fit hypersurface is found. Tests using both artificial and real data demonstrated the robustness of the method. As an illustration maps of deduced parameters of an emerging flux region are shown and briefly discussed.
Key words: techniques: polarimetric / methods: data analysis / Sun: chromosphere / Sun: infrared / Sun: magnetic field
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.