SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network
Journal article, 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.
Solar atmosphere
Chromosphere
ALMA
Millimeter radiation
Author
S. Wedemeyer
Universitetet i Oslo
Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.
T. Bastian
National Radio Astronomy Observatory
R. Brajsa
Sveuciliste u Zagrebu, Geodetski fakultet
Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.
M. Barta
Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.
H. Hudson
University of Glasgow
University of California System
G. Fleishman
New Jersey Institute of Technology
M. Loukitcheva
Max Planck Institut fur Sonnensystemforschung
Saint Petersburg State University
B. Fleck
NASA Goddard Space Flight Center
E. P. Kontar
University of Glasgow
B. De Pontieu
Lockheed Martin Corporation
S. Tiwari
NASA Marshall Space Flight Center
Y. Kato
Universitetet i Oslo
R. Soler
Universitat de les Illes Balears
P. Yagoubov
European Southern Observatory
John H Black
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
P. Antolin
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
S. Gunar
Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.
University of St Andrews
N. Labrosse
University of Glasgow
A.O. Benz
Fachhochschule Nordwestschweiz
A. Nindos
Panepistimion Ioanninon
M. Steffen
Astrophysikalisches Institut Potsdam
E. Scullion
Trinity College Dublin
J. G. Doyle
Armagh Observatory
T. Zaqarashvili
Institut fur Weltraumforschung
A. Hanslmeier
Karl-Franzens-Universitat Graz
V. M. Nakariakov
The University of Warwick
P. Heinzel
Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.
T. Ayres
University of Colorado at Boulder
M. Karlicky
Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.
Advances in Space Research
0273-1177 (ISSN)
Vol. 56 12 2679-2692Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
Roots
Basic sciences
Infrastructure
Onsala Space Observatory
DOI
10.1016/j.asr.2015.05.027