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


Wedemeyer, Sven; Bastian, Tim; Brajša, Roman; Barta, Miroslav; Hudson, Hugh; Fleishman, Gregory; Loukitcheva, Maria; Fleck, Bernhardt; Kontar, Eduard; DePontieu, Bart et al.
SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network // Advances in Space Research, 56 (2015), 12; 2679-2692 doi:10.1016/j.asr.2015.05.027 (međunarodna recenzija, članak, znanstveni)


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

Autori
Wedemeyer, Sven ; Bastian, Tim ; Brajša, Roman ; Barta, Miroslav ; Hudson, Hugh ; Fleishman, Gregory ; Loukitcheva, Maria ; Fleck, Bernhardt ; Kontar, Eduard ; DePontieu, Bart ; Tiwari, S. ; Kato, Y. ; Soler, R. ; Yagoubov, Pavel ; Black, J. H. ; Antolin, Patrick ; Gunar, S. ; Labrosse, Nicolas ; Benz, Arnold O. ; Nindos, A. ; Steffen, M. ; Scullion, E. ; Doyle, J. G. ; Zaqarashvili, Teimuraz ; Hanslmeier, Arnold ; Nakariakov, V. M. ; Heinzel, Petr ; Ayres, Tom ; Karlicky, Marian

Izvornik
Advances in Space Research (0273-1177) 56 (2015), 12; 2679-2692

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
solar atmosphere ; chromosphere ; millimeter radiation ; ALMA

Sažetak
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.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Ustanove
Geodetski fakultet, Zagreb

Profili:

Avatar Url Roman Brajša (autor)

Citiraj ovu publikaciju

Wedemeyer, Sven; Bastian, Tim; Brajša, Roman; Barta, Miroslav; Hudson, Hugh; Fleishman, Gregory; Loukitcheva, Maria; Fleck, Bernhardt; Kontar, Eduard; DePontieu, Bart et al.
SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network // Advances in Space Research, 56 (2015), 12; 2679-2692 doi:10.1016/j.asr.2015.05.027 (međunarodna recenzija, članak, znanstveni)
Wedemeyer, S., Bastian, T., Brajša, R., Barta, M., Hudson, H., Fleishman, G., Loukitcheva, M., Fleck, B., Kontar, E. & DePontieu, B. (2015) SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network. Advances in Space Research, 56 (12), 2679-2692 doi:10.1016/j.asr.2015.05.027.
@article{article, year = {2015}, pages = {2679-2692}, DOI = {10.1016/j.asr.2015.05.027}, keywords = {solar atmosphere, chromosphere, millimeter radiation, ALMA}, journal = {Advances in Space Research}, doi = {10.1016/j.asr.2015.05.027}, volume = {56}, number = {12}, issn = {0273-1177}, title = {SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network}, keyword = {solar atmosphere, chromosphere, millimeter radiation, ALMA} }

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • Science Citation Index Expanded (SCI-EXP)
    • SCI-EXP, SSCI i/ili A&HCI
  • Scopus


Uključenost u ostale bibliografske baze podataka:


  • NASA Astrophysics Data System


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