Number of the records: 1  

Velocity Vector, Ionization Degree, and Temperature of Prominence Fine Structures Observed by Hinode/SOT

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    SYSNO ASEP0386744
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleVelocity Vector, Ionization Degree, and Temperature of Prominence Fine Structures Observed by Hinode/SOT
    Author(s) Schmieder, B. (FR)
    Mein, P. (FR)
    Chandra, R. (FR)
    Molodij, G. (FR)
    Heinzel, Petr (ASU-R) RID, ORCID
    Berlicki, Arkadiusz (ASU-R) RID
    Schwartz, Pavol (ASU-R) RID
    Fárník, František (ASU-R) RID, ORCID
    Labrosse, N. (GB)
    Anzer, U. (DE)
    Watanabe, T. (JP)
    Source TitleHinode-3: The 3rd Hinode Science Meeting. - San Francisco : Astronomical Society otf the Pacific, 2012 / Sekii T. - ISBN 9781583817902
    Pagess. 107-112
    Number of pages6 s.
    Publication formPrint - P
    ActionHinode Science Meetin /3./
    Event date01.12.2009-04.12.2009
    VEvent locationTokyo
    CountryJP - Japan
    Event typeWRD
    Languageeng - English
    CountryUS - United States
    Keywordshedgerow prominence
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000312283700023
    AnnotationProminences have been successfully observed by Hinode in April 2007 exhibiting a strong dynamics of their fine structures. The dynamics of a prominence is a challenge to understand the formation of cool prominence plasma embedded in the hot corona. Combining simultaneous observations obtained in Hα with Hinode/SOT and the MSDP spectrograph operating at the Meudon solar tower, velocity vectors have been derived. The Doppler-shifts of bright threads are of the same order as the velocities measured perpendicular to the line of sight.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2013
Number of the records: 1  

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