Polarization Calibration of the Chromospheric Lyman-Alpha SpectroPolarimeter for a 0.1% Polarization Sensitivity in the VUV Range. Part II: In-Flight Calibration

G. Giono,R. Ishikawa, N. Narukage,R. Kano, Y. Katsukawa, M. Kubo,S. Ishikawa,T. Bando, H. Hara,Y. Suematsu, A. Winebarger, K. Kobayashi, F. Auchère,J. Trujillo Bueno, S. Tsuneta, T. Shimizu,T. Sakao, J. Cirtain, P. Champey,A. Asensio Ramos,J. Štěpán,L. Belluzzi,R. Manso Sainz,B. De Pontieu, K. Ichimoto, M. Carlsson, R. Casini, M. Goto

Solar Physics(2017)

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摘要
The Chromospheric Lyman-Alpha SpectroPolarimeter is a sounding rocket instrument designed to measure for the first time the linear polarization of the hydrogen Lyman- line (121.6 nm). The instrument was successfully launched on 3 September 2015 and observations were conducted at the solar disc center and close to the limb during the five-minutes flight. In this article, the disc center observations are used to provide an in-flight calibration of the instrument spurious polarization. The derived in-flight spurious polarization is consistent with the spurious polarization levels determined during the pre-flight calibration and a statistical analysis of the polarization fluctuations from solar origin is conducted to ensure a 0.014
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关键词
Polarization calibration,Vacuum ultraviolet,Lyman-alpha,Solar chromosphere,CLASP
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