Radiative Transfer in Stellar Atmospheres
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00355151" target="_blank" >RIV/67985815:_____/10:00355151 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Radiative Transfer in Stellar Atmospheres
Original language description
This review presents basic equations for the solution of the NLTE radiative transfer problem for trace elements and methods for its solution are summarized. The importance of frequency coupling in radiative transfer in stellar atmospheres is emphasized.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Non-LTE Line Formation for Trace Elements in Stellar Atmospheres
ISBN
9782759805884
ISSN
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e-ISSN
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Number of pages
18
Pages from-to
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Publisher name
EDP Sciences
Place of publication
Les Ulis
Event location
Nice
Event date
Jul 30, 2007
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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