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

0478693 - ASÚ 2018 NL eng J - Journal Article
Giono, G. - Ishikawa, R. - Narukage, N. - Kano, R. - Katsukawa, Y. - Kubo, M. - Ishikawa, S. - Bando, T. - Hara, H. - Suematsu, Y. - Winebarger, A. - Kobayashi, K. - Auchere, F. - Trujillo Bueno, J. - Tsuneta, S. - Shimizu, T. - Sakao, T. - Cirtain, J. - Champey, P. - Asensio Ramos, A. - Štěpán, Jiří - Belluzzi, L. - Sainz, R.M. - de Pontieu, B. - Ichimoto, K. - Carlsson, M. - Casini, R. - Goto, M.
Polarization Calibration of the Chromospheric Lyman-Alpha SpectroPolarimeter for a 0.1% Polarization Sensitivity in the VUV Range. Part II: In-Flight Calibration.
Solar Physics. Roč. 292, č. 4 (2017), 57/1-57/19. ISSN 0038-0938. E-ISSN 1573-093X
R&D Projects: GA ČR(CZ) GA16-16861S
Institutional support: RVO:67985815
Keywords : solar transition region * ly-alpha * magnetohydrodynamic model
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 2.580, year: 2017

The Chromospheric Lyman-Alpha SpectroPolarimeter is a sounding rocket instrument designed to measure for the first time the linear polarization of the hydrogen Lyman-alpha 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% precision on the spurious polarization. The combination of the pre-flight and the in-flight polarization calibrations provides a complete picture of the instrument response matrix, and a proper error transfer method is used to confirm the achieved polarization accuracy. As a result, the unprecedented 0.1% polarization accuracy of the instrument in the vacuum ultraviolet is ensured by the polarization calibration.
Permanent Link: http://hdl.handle.net/11104/0274753