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

Wedemeyer, S.; Bastian, T.S.; Brajša, R.; Hudson, H. S.; Fleishman, G.; Loukitcheva, M.; Fleck, B.; Kontar, E. P.; de Pontieu, B.; Yagoubov, P.; Tiwari, S.; Soler, R.; Black, J.H.; Antolin, P.; Scullion, E.; Gunár, Stanislav; Labrosse, N.; Ludwig, H.-G.; Benz, A. O.; White, S.M.; Hauschildt, P.; Doyle, J.G.; Nakariakov, V. M.; Ayres, T.; Heinzel, Petr; Karlický, Marian; Van Doorsselaere, T.; Gary, D.; Alissandrakis, C. E.; Nindos, A.; Solanki, S.K.; Rouppe van der Voort, L.; Shimojo, M.; Kato, Y.; Zaqarashvili, T.; Perez, E.; Selhorst, C.L.; Bárta, Miroslav

doi:https://dx.doi.org/10.1007/s11214-015-0229-9

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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, ORCID}
Source Title	Space Science Reviews. - : Springer - ISSN 0038-6308 Roč. 200, 1-4 (2016), s. 1-73
Number 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	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	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2017

Number of the records: 1