The effect of horizontal plasma inhomogeneities in 3D NLTE radiation 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_____%2F19%3A00517155" target="_blank" >RIV/67985815:_____/19:00517155 - isvavai.cz</a>
Alternative codes found
RIV/00216224:14310/19:00107435
Result on the web
<a href="https://doi.org/10.1016/j.jqsrt.2018.12.024" target="_blank" >https://doi.org/10.1016/j.jqsrt.2018.12.024</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.jqsrt.2018.12.024" target="_blank" >10.1016/j.jqsrt.2018.12.024</a>
Alternative languages
Result language
angličtina
Original language name
The effect of horizontal plasma inhomogeneities in 3D NLTE radiation transfer in stellar atmospheres
Original language description
We aim to demonstrate the effect of atmospheric inhomogeneities on the emergent specific intensity and radiation flux of a spectral line radiation. We self-consistently solve the NLTE problem for a two-level atom in a 3D atmosphere using the Cartesian grid. For that purpose, we use the 3D radiative transfer code PORTA. By examining simple examples, we study cases where the temperature inhomogeneities in the atmosphere models lead to the modification of the emergent radiation. We show that specific temperature inhomogeneities in the model atmospheres influence the emerging radiation, and that interpretation of the stellar spectra based on a plane-parallel atmosphere models can lead to erroneous conclusions about the atmospheric structure. (C) 2018 Elsevier Ltd. All rights reserved.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA16-01116S" target="_blank" >GA16-01116S: Atmospheres and circumstellar environment of magnetic hot stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Journal of Quantitative Spectroscopy and Radiative Transfer
ISSN
0022-4073
e-ISSN
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Volume of the periodical
225
Issue of the periodical within the volume
March
Country of publishing house
GB - UNITED KINGDOM
Number of pages
9
Pages from-to
249-257
UT code for WoS article
000460495100023
EID of the result in the Scopus database
2-s2.0-85059751044