Is it possible to model observed active region coronal emission simultaneously in EUV and X-ray filters?

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00364785" target="_blank" >RIV/67985815:_____/11:00364785 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201015947" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201015947</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201015947" target="_blank" >10.1051/0004-6361/201015947</a>

Result language
angličtina
Original language name
Is it possible to model observed active region coronal emission simultaneously in EUV and X-ray filters?
Original language description
We investigate the possibility of modeling the active region coronal emission in the EUV and X-ray filters using one, universal, steady heating function, tied to the properties of the magnetic field.
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
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Result description