SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network

Wedemeyer, S.; Bastian, T.S.; Brajsa, R.; Bárta, Miroslav; Hudson, H. S.; Fleishman, G.; Loukitcheva, M.; Fleck, B.; Kontar, E.; de Pontieu, B.; Tiwari, S.; Kato, Y.; Soler, R.; Yagoubov, P.; Black, J.H.; Antolin, P.; Gunár, Stanislav; Labrosse, N.; Benz, A. O.; Nindos, A.; Steffen, M.; Scullion, E.; Doyle, J.G.; Zaqarashvili, T.; Hanslmeier, A.; Nakariakov, V. M.; Heinzel, Petr; Ayres, T.; Karlický, Marian

doi:https://dx.doi.org/10.1016/j.asr.2015.05.027

Počet záznamů: 1

SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network

1.

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, ORCID}
Zdroj.dok.	Advances in Space Research. - : Elsevier - ISSN 0273-1177 Roč. 56, č. 12 (2015), s. 2679-2692
Poč.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