Stokes polarimetry at near-infrared 1.56 um for solar observation

Details Stokes polarimetry at near-infrared 1.56 um for solar observation Stokes polarimetry at near-infrared 1.56 um for solar observation

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002spie.4480..176c&link_type=abstract

Proc. SPIE Vol. 4480, p. 176-185, Imaging Spectrometry VII, Michael R. Descour; Sylvia S. Shen; Eds.

Physics

Scientific paper

FeI 1.56 micrometers Zeeman-sensitive lines are very important and potential to measure the magnetic field of the deepest layer of the solar photosphere. The new generation polarimeter is designed and manufactured in this wavelength range. By use of the polarimeter mounted on the vertical spectrograph of the 2m solar telescope at Kitt Peak, we can observe the Stokes I, Q, U, Vv parameters simultaneously. The paper presents the introduction of the near infrared polarimeter and the polarmetry of a sunspot group.

Affiliated with

Also associated with

No associations

Rating

Stokes polarimetry at near-infrared 1.56 um for solar observation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Stokes polarimetry at near-infrared 1.56 um for solar observation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stokes polarimetry at near-infrared 1.56 um for solar observation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1688475