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Infrared Stokes Polarimeter at NAOJ/Mitaka

Published online by Cambridge University Press:  06 January 2014

Yoichiro Hanaoka ,
Takashi Sakurai  and
IRMag Group
Yoichiro Hanaoka
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan email: hanaoka@solar.mtk.nao.ac.jp
Takashi Sakurai
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan email: hanaoka@solar.mtk.nao.ac.jp
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Abstract

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We have been operating an infrared Stokes spectro-polarimeter, whose observing wavelength bands include the He i 10830 Å and Fe i 15648 Å lines. A couple of full-Sun, full-Stokes maps in both wavelength bands are taken on a daily basis, with the polarization sensitivity better than 10−3. With this sensitivity, the helium polarization maps clearly show the atomic and Hanlé polarizations besides the Zeeman polarization, particularly in prominences/filaments. On these polarization maps, we can track the magnetic field signals of the prominences/filaments during their passages on the solar disk. Therefore, this instrument works as a ‘synoptic prominence magnetograph’. Our preliminary study of the linear polarizations seen in quiescent filaments suggests that the magnetic field producing the polarization signals is located at the bottom part of a flux-rope, which supports a filament.

Keywords

PolarimetryProminencesMagnetic Field
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 515 - 516
Copyright
Copyright © International Astronomical Union 2013 

References

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