Počet záznamů: 1
Solar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun
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SYSNO ASEP 0488872 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Solar 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, ORCID
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, ORCIDZdroj.dok. Space Science Reviews. - : Springer - ISSN 0038-6308
Roč. 200, 1-4 (2016), s. 1-73Poč.str. 73 s. Forma vydání Tištěná - P Jazyk dok. eng - angličtina Země vyd. NL - Nizozemsko Klíč. slova Sun ; photosphere ; chromosphere Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Obor OECD Astronomy (including astrophysics,space science) CEP 7E13003 GA MŠMT - Ministerstvo školství, mládeže a tělovýchovy LM2015067 GA MŠMT - Ministerstvo školství, mládeže a tělovýchovy UT WOS 000376077700001 EID SCOPUS 84951763921 DOI 10.1007/s11214-015-0229-9 Anotace The 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. Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2018
Počet záznamů: 1