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Solar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun
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SYSNO ASEP 0462727 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Solar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun Author(s) 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, ORCIDSource Title Space Science Reviews. - : Springer - ISSN 0038-6308
Roč. 200, 1-4 (2016), s. 1-73Number of pages 73 s. Publication form Print - P Language eng - English Country NL - Netherlands Keywords Sun ; photosphere ; chromosphere Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GA13-24782S GA ČR - Czech Science Foundation (CSF) Institutional support ASU-R - RVO:67985815 UT WOS 000376077700001 EID SCOPUS 84951763921 DOI https://doi.org/10.1007/s11214-015-0229-9 Annotation 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. Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2017
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