Dynamics of quiescent prominence fine structures analyzed by 2D non-LTE modelling of the H? line
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386855" target="_blank" >RIV/67985815:_____/12:00386855 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201218940" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201218940</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201218940" target="_blank" >10.1051/0004-6361/201218940</a>
Alternative languages
Result language
angličtina
Original language name
Dynamics of quiescent prominence fine structures analyzed by 2D non-LTE modelling of the H? line
Original language description
The combination of 2D non-LTE prominence fine-structure modelling with the statistical analysis of the observed and synthetic Lyman and H? spectra allows us to analyze the influence of the model input parameters and the velocity fields on the synthetic H? line profiles, thus determine the overall dynamics of the observed prominence as well as the physical parameters of its plasma.
Czech name
—
Czech description
—
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
—
Result continuities
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
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
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
—
Volume of the periodical
543
Issue of the periodical within the volume
July
Country of publishing house
FR - FRANCE
Number of pages
15
Pages from-to
"A93/1"-"A93/15"
UT code for WoS article
000306597200093
EID of the result in the Scopus database
—