Magnetic field strength of active region filaments

C. Kuckein, R. Centeno, V. Martínez Pillet, R. Casini, R. Manso Sainz, T. Shimizu

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66 Scopus citations

Abstract

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 10â ‰ 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.

Original languageEnglish
Pages (from-to)1113-1121
Number of pages9
JournalAstronomy and Astrophysics
Volume501
Issue number3
DOIs
StatePublished - 2009

Keywords

  • Sun: chromosphere
  • Sun: filaments
  • Sun: magnetic fields
  • Sun: photosphere
  • Techniques: polarimetric

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