Počet záznamů: 1
SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network
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SYSNO ASEP 0488863 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network Tvůrce(i) Wedemeyer, S. (NO)
Bastian, T.S. (US)
Brajsa, R. (NO)
Bárta, Miroslav (ASU-R) RID, ORCID
Hudson, H. S. (US)
Fleishman, G. (US)
Loukitcheva, M. (RU)
Fleck, B. (US)
Kontar, E. (GB)
de Pontieu, B. (US)
Tiwari, S. (US)
Kato, Y. (NO)
Soler, R. (ES)
Yagoubov, P. (DE)
Black, J.H. (SE)
Antolin, P. (JP)
Gunár, Stanislav (ASU-R) RID, ORCID
Labrosse, N. (GB)
Benz, A. O. (CH)
Nindos, A. (GR)
Steffen, M. (DE)
Scullion, E. (IE)
Doyle, J.G. (GB)
Zaqarashvili, T. (AT)
Hanslmeier, A. (AT)
Nakariakov, V. M. (GB)
Heinzel, Petr (ASU-R) RID, ORCID
Ayres, T. (US)
Karlický, Marian (ASU-R) RID, ORCIDZdroj.dok. Advances in Space Research. - : Elsevier - ISSN 0273-1177
Roč. 56, č. 12 (2015), s. 2679-2692Poč.str. 14 s. Forma vydání Tištěná - P Jazyk dok. eng - angličtina Země vyd. GB - Velká Británie Klíč. slova solar atmosphere ; chromosphere ; millimeter radiation 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 UT WOS 000366768200002 DOI 10.1016/j.asr.2015.05.027 Anotace The Solar Simulations for the Atacama Large Millimeter Observatory Network (SSALMON) was initiated in 2014 in connection with two ALMA development studies. The Atacama Large Millimeter/submillimeter Array (ALMA) is a powerful new tool, which can also observe the Sun at high spatial, temporal, and spectral resolution. The international SSALMONetwork aims at co-ordinating the further development of solar observing modes for ALMA and at promoting scientific opportunities for solar physics with particular focus on numerical simulations, which can provide important constraints for the observing modes and can aid the interpretation of future observations. The radiation detected by ALMA originates mostly in the solar chromosphere a complex and dynamic layer between the photosphere and corona, which plays an important role in the transport of energy and matter and the heating of the outer layers of the solar atmosphere. Potential targets include active regions, prominences, quiet Sun regions, flares Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2018
Počet záznamů: 1