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Doppler dimming and brightening effects in solar prominences

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00617195" target="_blank" >RIV/67985815:_____/24:00617195 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0364147" target="_blank" >https://hdl.handle.net/11104/0364147</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnrasl/slae055" target="_blank" >10.1093/mnrasl/slae055</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Doppler dimming and brightening effects in solar prominences

  • Original language description

    We explored the impact that Doppler dimming and brightening effects from bulk motions of solar prominences have on the formation of Ly α, H α, and Mg II h line profiles. We compared two schemes in which these effects manifest, when the prominence is moving radially away from the solar surface (radial case), and when the prominence is moving parallel to the solar surface (horizontal case). To do this, we analysed 13 332 model profiles generated through the use of the 1D NLTE (i.e. departures from Local Thermodynamic equilibrium) radiative transfer (RT) code PROMWEAVER, built on the LIGHTWEAVER NLTE RT framework to mimic the behaviour and output of the 1D NLTE RT code PROM. We found that horizontal velocities are just as, or more important than radial velocities. This demonstrates that horizontal velocities need to be accounted for when attempting to do any sort of forward modelling.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>SC</sub> - Article in a specialist periodical, which is included in the SCOPUS database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA22-34841S" target="_blank" >GA22-34841S: Science with Solar Orbiter: Focusing on eruptive processes</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society: Letters

  • ISSN

    1745-3925

  • e-ISSN

    1745-3933

  • Volume of the periodical

    533

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    6

  • Pages from-to

    "L19"-"L24"

  • UT code for WoS article

  • EID of the result in the Scopus database

    2-s2.0-85197872658