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

  1. 1.
    SYSNO ASEP0478693
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVZáznam nebyl označen do RIV
    Poddruh JČlánek ve WOS
    NázevPolarization 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 autorů28
    Zdroj.dok.Solar Physics. - : Springer - ISSN 0038-0938
    Roč. 292, č. 4 (2017), 57/1-57/19
    Poč.str.19 s.
    Forma vydáníTištěná - P
    Jazyk dok.eng - angličtina
    Země vyd.NL - Nizozemsko
    Klíč. slovasolar transition region ; ly-alpha ; magnetohydrodynamic model
    Vědní obor RIVBN - Astronomie a nebeská mechanika, astrofyzika
    Obor OECDAstronomy (including astrophysics,space science)
    CEPGA16-16861S GA ČR - Grantová agentura ČR
    Institucionální podporaASU-R - RVO:67985815
    UT WOS000399832600012
    EID SCOPUS85016727277
    DOI10.1007/s11207-017-1062-y
    AnotaceThe 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.
    PracovištěAstronomický ústav
    KontaktRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Rok sběru2018
Počet záznamů: 1  

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