期刊
ADVANCES IN SPACE RESEARCH
卷 56, 期 12, 页码 2679-2692出版社
ELSEVIER SCI LTD
DOI: 10.1016/j.asr.2015.05.027
关键词
Solar atmosphere; Chromosphere; Millimeter radiation; ALMA
类别
资金
- Faculty of Mathematics and Natural Sciences of the University of Oslo, Norway
- Research Council of Norway [221767/F20]
- European Commission through the CIG Grant [PCIG-GA-2011-304265]
- European Commission through the GACR Grant [13-24782S]
- European Commission eHEROES [284461]
- European Commission SOLARNET [312495]
- Croatian Science Foundation [6212]
- Marie Curie Radio Sun project [PIRSES-GA-2011-295272]
- NSF [AGS-1250374, AGS-1262772]
- NASA [NNX14AC87G]
- Saint Petersburg State University [6.0.26.2010, 6.37.343.2015]
- RFBR [15-02-03835]
- European Union (European Social Fund-ESF)
- Greek national funds through the Operational Program Education and Lifelong Learning of the National Strategic Reference Framework (NSRF) Research Funding Program: Thales
- Austrian Science Fund (FWF) [P 26181] Funding Source: researchfish
- Div Atmospheric & Geospace Sciences
- Directorate For Geosciences [1262772, 1250374] Funding Source: National Science Foundation
- STFC [ST/L000741/1] Funding Source: UKRI
- Austrian Science Fund (FWF) [P26181] Funding Source: Austrian Science Fund (FWF)
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. Here, we give a brief overview over the network and potential science cases for future solar observations with ALMA. (C) 2015 COSPAR. Published by Elsevier Ltd. All rights reserved.
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