Počet záznamů: 1
Polarization Calibration of the Chromospheric Lyman-Alpha SpectroPolarimeter for a 0.1% Polarization Sensitivity in the VUV Range. Part II: In-Flight Calibration
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SYSNO ASEP 0478693 Druh ASEP J - Článek v odborném periodiku Zařazení RIV Záznam nebyl označen do RIV Poddruh J Článek ve WOS Název Polarization Calibration of the Chromospheric Lyman-Alpha SpectroPolarimeter for a 0.1% Polarization Sensitivity in the VUV Range. Part II: In-Flight Calibration Tvůrce(i) Giono, G. (JP)
Ishikawa, R. (JP)
Narukage, N. (JP)
Kano, R. (JP)
Katsukawa, Y. (JP)
Kubo, M. (JP)
Ishikawa, S. (JP)
Bando, T. (JP)
Hara, H. (JP)
Suematsu, Y. (JP)
Winebarger, A. (US)
Kobayashi, K. (JP)
Auchere, F. (FR)
Trujillo Bueno, J. (ES)
Tsuneta, S. (JP)
Shimizu, T. (JP)
Sakao, T. (US)
Cirtain, J. (US)
Champey, P. (FR)
Asensio Ramos, A. (ES)
Štěpán, Jiří (ASU-R) RID, ORCID
Belluzzi, L. (ES)
Sainz, R.M. (ES)
de Pontieu, B. (US)
Ichimoto, K. (JP)
Carlsson, M. (SE)
Casini, R. (US)
Goto, M. (JP)Celkový počet autorů 28 Zdroj.dok. Solar Physics. - : Springer - ISSN 0038-0938
Roč. 292, č. 4 (2017), 57/1-57/19Poč.str. 19 s. Forma vydání Tištěná - P Jazyk dok. eng - angličtina Země vyd. NL - Nizozemsko Klíč. slova solar transition region ; ly-alpha ; magnetohydrodynamic model Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Obor OECD Astronomy (including astrophysics,space science) CEP GA16-16861S GA ČR - Grantová agentura ČR Institucionální podpora ASU-R - RVO:67985815 UT WOS 000399832600012 EID SCOPUS 85016727277 DOI 10.1007/s11207-017-1062-y Anotace 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. Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2018
Počet záznamů: 1