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Solar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun

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    SYSNO ASEP0462727
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevSolar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun
    Tvůrce(i) Wedemeyer, S. (NO)
    Bastian, T.S. (US)
    Brajša, R. (HR)
    Hudson, H. S. (US)
    Fleishman, G. (US)
    Loukitcheva, M. (RU)
    Fleck, B. (US)
    Kontar, E. P. (GB)
    de Pontieu, B. (US)
    Yagoubov, P. (DE)
    Tiwari, S. (US)
    Soler, R. (ES)
    Black, J.H. (SE)
    Antolin, P. (JP)
    Scullion, E. (IE)
    Gunár, Stanislav (ASU-R) RID, ORCID
    Labrosse, N. (FR)
    Ludwig, H.-G. (DE)
    Benz, A. O. (CH)
    White, S.M. (US)
    Hauschildt, P. (DE)
    Doyle, J.G. (GB)
    Nakariakov, V. M. (GB)
    Ayres, T. (US)
    Heinzel, Petr (ASU-R) RID
    Karlický, Marian (ASU-R) RID, ORCID
    Van Doorsselaere, T. (BE)
    Gary, D. (US)
    Alissandrakis, C. E. (GR)
    Nindos, A. (GR)
    Solanki, S.K. (DE)
    Rouppe van der Voort, L. (NO)
    Shimojo, M. (JP)
    Kato, Y. (NO)
    Zaqarashvili, T. (AT)
    Perez, E. (GB)
    Selhorst, C.L. (BR)
    Bárta, Miroslav (ASU-R) RID, ORCID
    Zdroj.dok.Space Science Reviews - ISSN 0038-6308
    Roč. 200, 1-4 (2016), s. 1-73
    Poč.str.73 s.
    Forma vydáníTištěná - P
    Jazyk dok.eng - angličtina
    Země vyd.NL - Nizozemsko
    Klíč. slovaSun ; photosphere ; chromosphere
    Vědní obor RIVBN - Astronomie a nebeská mechanika, astrofyzika
    CEPGA13-24782S GA ČR - Grantová agentura ČR
    Institucionální podporaASU-R - RVO:67985815
    UT WOS000376077700001
    EID SCOPUS84951763921
    DOI10.1007/s11214-015-0229-9
    AnotaceThe Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can address a broad range of fundamental scientific questions in solar physics. The radiation observed by ALMA originates mostly from the chromosphere-a complex and dynamic region between the photosphere and corona, which plays a crucial role in the transport of energy and matter and, ultimately, the heating of the outer layers of the solar atmosphere. Based on first solar test observations, strategies for regular solar campaigns are currently being developed. State-of-the-art numerical simulations of the solar atmosphere and modeling of instrumental effects can help constrain and optimize future observing modes for ALMA. Here we present a short technical description of ALMA and an overview of past efforts and future possibilities for solar observations at submillimeter and millimeter wavelengths. In addition, selected numerical simulations and observations at other wavelengths demonstrate ALMA's scientific potential for studying the Sun for a large range of science cases.
    PracovištěAstronomický ústav
    KontaktRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Rok sběru2017
Počet záznamů: 1