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.

Solar atmosphere

Chromosphere

ALMA

Millimeter radiation

Författare

S. Wedemeyer

Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.

Universitetet i Oslo

T. Bastian

National Radio Astronomy Observatory

R. Brajsa

Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.

Sveuciliste u Zagrebu, Geodetski fakultet

M. Barta

Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i.

H. Hudson

University of Glasgow

University of California

G. Fleishman

New Jersey Institute of Technology

M. Loukitcheva

Saint Petersburg State University - Spsu

Max Planck-institutet

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 (ESO)

John H Black

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

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

Panepistimio 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-Universität 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 2679-2692

Ämneskategorier

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

Infrastruktur

Onsala rymdobservatorium

DOI

10.1016/j.asr.2015.05.027