On the nature of pronimence emission observed by SDO/AIA
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386866" target="_blank" >RIV/67985815:_____/12:00386866 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/0004-637X/754/1/66" target="_blank" >http://dx.doi.org/10.1088/0004-637X/754/1/66</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/0004-637X/754/1/66" target="_blank" >10.1088/0004-637X/754/1/66</a>
Alternative languages
Result language
angličtina
Original language name
On the nature of pronimence emission observed by SDO/AIA
Original language description
We investigate the temperature sensitivity of these AIA bands for prominence observations, in order to infer the temperature content in an effort to explain the emission. Using the CHIANTI atomic database and previously determined prominence differentialemission measure distributions, we build synthetic spectra to establish the main emission-line contributors in the AIA bands.
Czech name
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Czech description
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Classification
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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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysical Journal
ISSN
0004-637X
e-ISSN
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Volume of the periodical
754
Issue of the periodical within the volume
1
Country of publishing house
US - UNITED STATES
Number of pages
8
Pages from-to
"66/1"-"66/8"
UT code for WoS article
000306111800066
EID of the result in the Scopus database
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