SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network
Artikel i vetenskaplig tidskrift, 2015
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.
Millimeter radiation
Solar atmosphere
ALMA
Chromosphere
Författare
S. Wedemeyer
Czech Academy of Sciences
Universitetet i Oslo
T. Bastian
National Radio Astronomy Observatory
R. Brajsa
Sveučilište u Zagrebu
Czech Academy of Sciences
M. Barta
Czech Academy of Sciences
H. Hudson
University of Glasgow
University of California
G. Fleishman
New Jersey Institute of Technology
M. Loukitcheva
Saint Petersburg State University - Spsu
Max-Planck-Gesellschaft
B. Fleck
National Aeronautics and Space Administration (NASA)
E. P. Kontar
University of Glasgow
B. De Pontieu
Lockheed Martin Corporation
S. Tiwari
National Aeronautics and Space Administration (NASA)
Y. Kato
Universitetet i Oslo
R. Soler
Universitat de les Illes Balears
P. Yagoubov
European Southern Observatory (ESO)
John H Black
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
P. Antolin
National Astronomical Observatory of Japan
S. Gunar
Czech Academy of Sciences
University of St Andrews
N. Labrosse
University of Glasgow
A.O. Benz
Fachhochschule Nordwestschweiz
A. Nindos
University of Ioannina
M. Steffen
Leibniz-Institut Für Astrophysik Potsdam
E. Scullion
Trinity College Dublin
J. G. Doyle
Armagh Observatory and Planetarium
T. Zaqarashvili
Institut fur Weltraumforschung
A. Hanslmeier
Karl-Franzens-Universität Graz
V. M. Nakariakov
The University of Warwick
P. Heinzel
Czech Academy of Sciences
T. Ayres
University of Colorado at Boulder
M. Karlicky
Czech Academy of Sciences
Advances in Space Research
0273-1177 (ISSN) 18791948 (eISSN)
Vol. 56 12 2679-2692Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
Infrastruktur
Onsala rymdobservatorium
DOI
10.1016/j.asr.2015.05.027