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Solar Research with ALMA
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SYSNO ASEP 0353878 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Solar Research with ALMA Author(s) Karlický, Marian (ASU-R) RID, ORCID
Bárta, Miroslav (ASU-R) RID, ORCID
Dabrowski, Bartosz Premyslaw (ASU-R) RID
Heinzel, Petr (ASU-R) RID, ORCIDSource Title Solar Physics. - : Springer - ISSN 0038-0938
Roč. 268, č. 1 (2011), s. 165-173Number of pages 9 s. Language eng - English Country NL - Netherlands Keywords Sun ; atmosphere ; radio radiation ; radioheliograph Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects IAA300030701 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) GAP209/10/1680 GA ČR - Czech Science Foundation (CSF) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000285364400007 DOI 10.1007/s11207-010-9671-8 Annotation The Atacama Large Millimeter/sub-millimeter Array (ALMA) is a large interferometer that will consist up to 64 high-precision antennas operating in the 31.3 - 950 GHz frequency range. In this frequency range, which is largely unexplored, unique observations with a broad range of scientific objectives are expected. Among these tasks there is a unique possibility to observe the Sun and to address several outstanding issues of solar physics. The ALMA is briefly described and then the new ESO-ALMA European node (ARC), built at Ondřejov Observatory, is presented. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2011
Number of the records: 1