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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

  • DOI - Digital Object Identifier

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

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

  • 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

  • e-ISSN

  • Number of pages

    18

  • Pages from-to

  • 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