Bibcode
Kuckein, C.; Centeno, R.; Martínez Pillet, V.; Casini, R.; Manso Sainz, R.; Shimizu, T.
Bibliographical reference
Astronomy and Astrophysics, Volume 501, Issue 3, 2009, pp.1113-1121
Advertised on:
7
2009
Journal
Citations
75
Refereed citations
58
Description
Aims: We study the vector magnetic field of a filament observed over a
compact active region neutral line. Methods: Spectropolarimetric
data acquired with TIP-II (VTT, Tenerife, Spain) of the 10 830 Å
spectral region provide full Stokes vectors that were analyzed using
three different methods: magnetograph analysis, Milne-Eddington
inversions, and PCA-based atomic polarization inversions. Results: The inferred magnetic field strengths in the filament are
around 600-700 G by all these three methods. Longitudinal fields are
found in the range of 100-200 G whereas the transverse components become
dominant, with fields as high as 500-600 G. We find strong transverse
fields near the neutral line also at photospheric levels. Conclusions: Our analysis indicates that strong (higher than 500 G,
but below kG) transverse magnetic fields are present in active region
filaments. This corresponds to the highest field strengths reliably
measured in these structures. The profiles of the helium 10 830 Å
lines observed in this active region filament are dominated by the
Zeeman effect.
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