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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

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • 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

  • 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