Optical-to-Radio Continua in Solar Flares

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386857" target="_blank" >RIV/67985815:_____/12:00386857 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11207-011-9823-5" target="_blank" >http://dx.doi.org/10.1007/s11207-011-9823-5</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-011-9823-5" target="_blank" >10.1007/s11207-011-9823-5</a>

Result language
angličtina
Original language name
Optical-to-Radio Continua in Solar Flares
Original language description
Spectral continua observed during solar flares may contain information about both thermal and non-thermal heating mechanisms. Using two semi-empirical flare models F2 and FLA, we synthesize the thermal continua from optical to mm?radio domains and compare their intensities with quiet-Sun values computed from a recent model C7. In this way, the far-infrared and sub-mm/mm continua are studied for the first time, and we present our results as a benchmark for further modeling and for planning new observations, especially with the ALMA instrument. Finally, we demonstrate how these continua are formed and show a close correspondence between their brightness temperature and the kinetic-temperature structure of the flaring atmosphere.
Czech name
—
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
<a href="/en/project/GAP209%2F10%2F1680" target="_blank" >GAP209/10/1680: Energetic Processes In Solar Atmosphere: Relations of Simulations to Observations</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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