Solar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00462727" target="_blank" >RIV/67985815:_____/16:00462727 - isvavai.cz</a>
Alternative codes found
RIV/67985815:_____/16:00488872
Result on the web
<a href="http://dx.doi.org/10.1007/s11214-015-0229-9" target="_blank" >http://dx.doi.org/10.1007/s11214-015-0229-9</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11214-015-0229-9" target="_blank" >10.1007/s11214-015-0229-9</a>

Result language
angličtina
Original language name
Solar Science with the Atacama Large Millimeter/Submillimeter Array-A New View of Our Sun
Original language description
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.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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