| Full text | |
| Author(s): Show less - |
Wedemeyer, S.
[1, 2]
;
Bastian, T.
[3]
;
Brajsa, R.
[2, 4]
;
Hudson, H.
[5, 6]
;
Fleishman, G.
[7]
;
Loukitcheva, M.
[8, 9]
;
Fleck, B.
[10]
;
Kontar, E. P.
[5]
;
De Pontieu, B.
[1, 11]
;
Yagoubov, P.
[12]
;
Tiwari, S. K.
[13]
;
Soler, R.
[14]
;
Black, J. H.
[15]
;
Antolin, P.
[16]
;
Scullion, E.
[17]
;
Gunar, S.
[18, 19]
;
Labrosse, N.
[5]
;
Ludwig, H. -G.
[20]
;
Benz, A. O.
[21]
;
White, S. M.
[22]
;
Hauschildt, P.
[23]
;
Doyle, J. G.
[24]
;
Nakariakov, V. M.
[25]
;
Ayres, T.
[26]
;
Heinzel, P.
[19]
;
Karlicky, M.
[19]
;
Van Doorsselaere, T.
[27]
;
Gary, D.
[7]
;
Alissandrakis, C. E.
[28]
;
Nindos, A.
[28]
;
Solanki, S. K.
[8, 29]
;
van der Voort, L. Rouppe
[1]
;
Shimojo, M.
[16]
;
Kato, Y.
[1]
;
Zaqarashvili, T.
[30, 31]
;
Perez, E.
[5]
;
Selhorst, C. L.
[32]
;
Barta, M.
[19, 2]
Total Authors: 38
|
| Affiliation: Show less - | [1] Univ Oslo, Inst Theoret Astrophys, Postboks 1029, N-0315 Oslo - Norway
[2] ASCR, Astron Inst, Czech Node, European ARC, Ondrejov - Czech Republic
[3] NRAO, 520 Edgemont Rd, Charlottesville, VA 22903 - USA
[4] Univ Zagreb, Fac Geodesy, Hvar Observ, Zagreb 41000 - Croatia
[5] Univ Glasgow, Sch Phys & Astron, SUPA, Glasgow G12 8QQ, Lanark - Scotland
[6] Univ Calif Berkeley, Space Sci Lab, 7 Gauss Way, Berkeley, CA 94720 - USA
[7] New Jersey Inst Technol, Dept Phys, Ctr Solar Terr Res, 323 MLK Blvd, Newark, NJ 07102 - USA
[8] Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen - Germany
[9] St Petersburg Univ, Astron Inst, Univ Skii Pr 28, St Petersburg 198504 - Russia
[10] NASA, ESA Sci Operat Dept, Goddard Space Flight Ctr, Greenbelt, MD - USA
[11] Lockheed Martin Solar & Astrophys Lab, 3251 Hanover St, Org A021S, B-252, Palo Alto, CA 94304 - USA
[12] European Org Astron Res Southern Hemisphere ESO, Karl Schwarzschild Str 2, D-85748 Garching - Germany
[13] NASA, Marshall Space Flight Ctr, ZP 13, Huntsville, AL 35805 - USA
[14] Univ Illes Balears, Dept Fis, Palma De Mallorca 07122 - Spain
[15] Chalmers, Onsala Space Observ, Dept Earth & Space Sci, S-43992 Onsala - Sweden
[16] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588 - Japan
[17] Univ Dublin Trinity Coll, Coll Green, Dublin 2 - Ireland
[18] Univ St Andrews, Sch Math & Stat, St Andrews KY16 9SS, Fife - Scotland
[19] Acad Sci Czech Republic, Astron Inst, Fricova 298, Ondrejov 25165 - Czech Republic
[20] ZAH, Landessternwarte Konigstuhl 12, D-69117 Heidelberg - Germany
[21] FHNW, Inst Technol 4D, Windisch - Switzerland
[22] AFRL, Space Vehicles Directorate, 3550 Aberdeen Ave SE, Bldg 427, Kirtland AFB, NM 87117 - USA
[23] Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg - Germany
[24] Coll Hill, Armagh Observ, Armagh BT61 9DG - North Ireland
[25] Univ Warwick, Dept Phys, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands - England
[26] Univ Colorado, Ctr Astrophys & Space Astron, Campus Box 391, Boulder, CO 80309 - USA
[27] Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, Celestijnenlaan 200B Bus 2400, B-3000 Leuven - Belgium
[28] Univ Ioannina, Dept Phys, POB 1186, GR-45110 Ioannina - Greece
[29] Kyung Hee Univ, Sch Space Res, Yongin, Gyeonggi - South Korea
[30] Graz Univ, Inst Phys, Univ Pl 5, A-8010 Graz - Austria
[31] Ilia State Univ, Abastumani Astrophys Observ, Univ St 2, Tbilisi - Rep of Georgia
[32] Univ Vale Paraiba UNIVAP, Av Shishima Hifumi 2911, BR-12244000 Sao Jose Dos Campos, SP - Brazil
Total Affiliations: 32
|
| Document type: | Review article |
| Source: | SPACE SCIENCE REVIEWS; v. 200, n. 1-4, p. 1-73, APR 2016. |
| Web of Science Citations: | 35 |
| Abstract | |
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. (AU) | |
| FAPESP's process: | 14/10489-0 - Study of the changes in the solar magnetic field based on radio observations |
| Grantee: | Caius Lucius Selhorst |
| Support Opportunities: | Regular Research Grants |