Počet záznamů: 1

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

SYSNO ASEP	0462727
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, ORCID}
Zdroj.dok.	Space Science Reviews. - : Springer - ISSN 0038-6308 Roč. 200, 1-4 (2016), s. 1-73
Poč.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
CEP	GA13-24782S GA ČR - Grantová agentura ČR
Institucionální podpora	ASU-R - RVO:67985815
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	2017

Počet záznamů: 1