Pregled bibliografske jedinice broj: 807887
Solar Science with the Atacama Large Millimeter/Submillimeter Array - A New View of Our Sun
Solar Science with the Atacama Large Millimeter/Submillimeter Array - A New View of Our Sun // Space science reviews, 200 (2016), 1-4; 1-73 doi:10.1007/s11214-015-0229-9 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 807887 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Solar Science with the Atacama Large Millimeter/Submillimeter Array - A New View of Our Sun
Autori
Wedemeyer, Sven ; Bastian, Tim ; Brajša, Roman ; Hudson, Hugh ; Fleishman, Gregory ; Loukitcheva, Maria ; Fleck, Bernhardt ; Kontar, Eduard ; DePontieu, Bart ; Yagoubov, Pavel ; Tiwari, S. K. ; Soler, R. ; Black, J. H. ; Antolin, Patrick ; Scullion, E. ; Gunar, S. ; Labrosse, Nicolas ; Ludwig, H.-G. ; Benz, Arnold O. ; White, Stephen M. ; Hauschildt, P. ; Doyle, J. G. ; Nakariakov, V. M. ; Ayres, Tom ; Heinzel, Petr ; Karlicky, Marian ; Van Doorsselaere, T. ; Gary, Dale ; Alissandrakis, C. E. ; Nindos, A. ; Solanki, S. K. ; Rouppe van der Voort, L. ; Shimojo, M. ; Kato, Y. ; Zaqarashvili, Teimuraz ; Perez, E., Selhorst, C. L. ; Barta, Miroslav
Izvornik
Space science reviews (0038-6308) 200
(2016), 1-4;
1-73
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
Sun ; Photosphere ; Chromosphere ; Corona ; Magnetohydrodynamics ; Radiative transfer ; Flares ; Prominences
Sažetak
The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can address a broad range of fundamental scientific questions in solar physics. The radiation observed by ALMA originates mostly from the chromosphere—a complex and dynamic region between the photosphere and corona, which plays a crucial role in the transport of energy and matter and, ultimately, the heating of the outer layers of the solar atmosphere. Based on first solar test observations, strategies for regular solar campaigns are currently being developed. State-of-the-art numerical simulations of the solar atmosphere and modeling of instrumental effects can help constrain and optimize future observing modes for ALMA. Here we present a short technical description of ALMA and an overview of past efforts and future possibilities for solar observations at submillimeter and millimeter wavelengths. In addition, selected numerical simulations and observations at other wavelengths demonstrate ALMA’s scientific potential for studying the Sun for a large range of science cases.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
HRZZ-IP-2013-11-6212 - Promjenjivost Sunca i zvijezda (SOLSTEL) (Vršnak, Bojan, HRZZ - 2013-11) ( CroRIS)
Ustanove:
Geodetski fakultet, Zagreb
Profili:
Roman Brajša
(autor)
Citiraj ovu publikaciju:
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::
- INSPEC
- NASA ADS