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Fast approximate radiative transfer method for visualizing the fine structure of prominences in the hydrogen H alpha line

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00452509" target="_blank" >RIV/67985815:_____/15:00452509 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201525716" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201525716</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201525716" target="_blank" >10.1051/0004-6361/201525716</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Fast approximate radiative transfer method for visualizing the fine structure of prominences in the hydrogen H alpha line

  • Original language description

    We present a novel approximate radiative transfer method developed to visualize 3D whole-prominence models with multiple fine structures using the hydrogen H alpha spectral line. We provide recipes for the use of this method for visualizing the prominence or filament models that have multiple fine structures. We also perform tests of the method that demonstrate its accuracy under prominence conditions. We demonstrate that this fast approximate radiative transfer method provides realistic synthetic H alpha intensities useful for a reliable visualization of prominences and filaments. Such synthetic high-resolution images of modeled prominences/filaments can be used for a direct comparison with high-resolution observations.n

  • 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/GAP209%2F12%2F0906" target="_blank" >GAP209/12/0906: Realistic solar prominence models combining radiative transfer modeling and MHD simulatios</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2015

  • 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

    1432-0746

  • e-ISSN

  • Volume of the periodical

    579

  • Issue of the periodical within the volume

    July

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    6

  • Pages from-to

    "A16/1"-"A16/6"

  • UT code for WoS article

    000358877100028

  • EID of the result in the Scopus database