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Theoretical relations between model parameters and Metis observables for eruptive prominences and coronal mass ejections

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00619114" target="_blank" >RIV/67985815:_____/25:00619114 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0365901" target="_blank" >https://hdl.handle.net/11104/0365901</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202453116" target="_blank" >10.1051/0004-6361/202453116</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Theoretical relations between model parameters and Metis observables for eruptive prominences and coronal mass ejections

  • Original language description

    Context. We investigate the behavior of the plasma in eruptive prominences and coronal mass ejections in characteristic physical conditions. Aims. We aim to demonstrate various relations between the plasma parameters and radiation properties relevant to Solar Orbiter and Metis observations. Methods. Our method is based on 2D non-local thermodynamic equilibrium (non-LTE) modeling of moving structures that are externally illuminated from the solar disk. We have focused on temperatures below 105 K and a range of gas pressures to investigate the opacity effects in the L alpha line. Overall, we applied a large grid of isothermal and isobaric models. Results. Our results are presented in the form of various correlation plots showing relationships between the plasma parameters and radiation properties relevant to Metis observations. We also demonstrate the relative importance of radiative and collisional ionization of hydrogen and the ratio between radiative and collisional excitation of the L alpha line. Our results point to the need to carry out optically thick non-LTE modeling for specific plasma conditions. The visible light (VL) emission was also obtained for the purposes of a comparison with the Metis data.

  • 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

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    696

  • Issue of the periodical within the volume

    March

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    9

  • Pages from-to

    A14

  • UT code for WoS article

    001455406500002

  • EID of the result in the Scopus database

    2-s2.0-105001643801