Počet záznamů: 1  

A Sounding Rocket Experiment for the Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP)

  1. 1.
    SYSNO ASEP0435543
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleA Sounding Rocket Experiment for the Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP)
    Author(s) Kubo, M. (JP)
    Kano, R. (JP)
    Kobayashi, K. (JP)
    Bando, T. (JP)
    Narukage, N. (JP)
    Ishikawa, R. (JP)
    Tsuneta, S. (JP)
    Katsukawa, Y. (JP)
    Ishikawa, S. (JP)
    Suematsu, Y. (JP)
    Hara, H. (JP)
    Shimizu, T. (JP)
    Sakao, T. (US)
    Ichimoto, K. (JP)
    Goto, M. (JP)
    Holloway, T. (US)
    Winebarger, A. (US)
    Cirtain, J. (US)
    de Pontieu, B. (US)
    Casini, R. (US)
    Auchere, F. (FR)
    Trujillo Bueno, J. (ES)
    Manso Sainz, R. (ES)
    Belluzzi, L. (ES)
    AsensioRamos, A. (ES)
    Štěpán, Jiří (ASU-R) RID, ORCID
    Carlsson, M. (NO)
    Source TitleSolar Polarization 7. - San Francisco : Astronomical Society of the Pacific, 2014 / Nagendra K.N. - ISBN 9781583818633
    Pagess. 307-317
    Number of pages11 s.
    Publication formPrint - P
    ActionSolar Polarization 7
    Event date09.09.2013-13.09.2013
    VEvent locationKunning
    CountryCN - China
    Event typeWRD
    Languageeng - English
    CountryUS - United States
    Keywordsmagnetic fields ; polarization ; scattering
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGPP209/12/P741 GA ČR - Czech Science Foundation (CSF)
    Institutional supportASU-R - RVO:67985815
    UT WOS000370308600030
    AnnotationA sounding-rocket experiment called the Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) is presently under development to measure the linear polarization profiles in the hydrogen Lyman-alpha (Lyα) line at 121.567 nm. CLASP is a vacuum-UV (VUV) spectropolarimeter to aim for first detection of the linear polarizations caused by scattering processes and the Hanle effect in the Lyα line with high accuracy (0.1%). This is a fist step for exploration of magnetic fields in the upper chromosphere and transition region of the Sun. Accurate measurements of the linear polarization signals caused by scattering processes and the Hanle effect in strong UV lines like Lyα are essential to explore with future solar telescopes the strength and structures of the magnetic field in the upper chromosphere and transition region of the Sun. The CLASP proposal has been accepted by NASA in 2012, and the flight is planned in 2015.
    WorkplaceAstronomical Institute
    ContactAnežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2015
Počet záznamů: 1  

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