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Radiative transfer in Solar prominences: An overview and current trends

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00642907" target="_blank" >RIV/67985815:_____/25:00642907 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0372825" target="_blank" >https://hdl.handle.net/11104/0372825</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s11207-025-02585-y" target="_blank" >10.1007/s11207-025-02585-y</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Radiative transfer in Solar prominences: An overview and current trends

  • Original language description

    We review the development of the non-LTE (i.e. departures from Local Thermodynamic Equilibrium) radiative-transfer modeling of cool coronal condensations, namely solar prominences. The period considered covers five decades, but we particularly focus on current trends and advancements. Our main goal is to critically discuss various issues of the model geometries and how the assumed geometry couples to the specification of the incident illumination from the surrounding atmosphere. We start with initial one-dimensional (1D) models and continue with the discussion of 2D models and the current 3D approaches. A special attention is devoted to highly heterogeneous prominence structures and to fast-moving eruptive prominences currently well observed by the Metis and EUI instruments onboard Solar Orbiter and by the ASPIICS large coronagraph onboard the Proba-3 formation-flight mission.

  • 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/GA25-18282S" target="_blank" >GA25-18282S: ESA space coronagraphy with Czech participation</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Solar Physics

  • ISSN

    0038-0938

  • e-ISSN

    1573-093X

  • Volume of the periodical

    300

  • Issue of the periodical within the volume

    12

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    18

  • Pages from-to

    167

  • UT code for WoS article

    001624840100004

  • EID of the result in the Scopus database

    2-s2.0-105023215368