Share Email Print
cover

Proceedings Paper

Development of the high-resolution spectropolarimeter: LIPS
Author(s): Yuji Ikeda; Hiroshi Akitaya; Kentaro Matsuda; Koji S. Kawabata; Munezo Seki; Ryuko Hirata; Akira Okazaki
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

We are developing a Cassegrain optical spectropolarimeter, LIPS. LIPS employs an echelle-type spectrograph to get a high spectral resolution of R > 7,000. LIPS consists of three instrumental units, a polarimeter, a spectrometer, and a detector. One serious problem was the appearance of 'spectral ripple' generated in the Pancharatnam type super-achromatic half-wave plate (PWP). We found out through laboratory works and numerical simulations that the ripple is caused by the interference among layers in the half-wave plate. In stead of PWP, we adopted a new type of super-achromatic half-wave plate composed of five polymethyl-methacrylate layers, which was manufactured by Astropribor Company in Ukraine. This wave plate greatly reduces reflection at the boundaries among layers, which results in significant reduction of ripple. Since the spring of 2001, we have carried out engineering observations with LIPS at IRS and UH88. We conclude from these observations that LIPS have achieved the accuracy of ΔP < 0.1 %.

Paper Details

Date Published: 14 February 2003
PDF: 11 pages
Proc. SPIE 4843, Polarimetry in Astronomy, (14 February 2003); doi: 10.1117/12.458833
Show Author Affiliations
Yuji Ikeda, Genesia Corp. (United States)
Hiroshi Akitaya, Tohoku Univ. (United States)
Kentaro Matsuda, Tohoku Univ. (United States)
Koji S. Kawabata, National Astronomical Observatory of Japan (United States)
Munezo Seki, Tohoku Univ. (United States)
Ryuko Hirata, Kyoto Univ. (United States)
Akira Okazaki, Gunma Univ. (United States)


Published in SPIE Proceedings Vol. 4843:
Polarimetry in Astronomy
Silvano Fineschi, Editor(s)

© SPIE. Terms of Use
Back to Top