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Modeling of the solar flare chromosphere and sub-THz radiation with FLARIX and RADYN

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00616823" target="_blank" >RIV/67985815:_____/24:00616823 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921323005276" target="_blank" >http://dx.doi.org/10.1017/S1743921323005276</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921323005276" target="_blank" >10.1017/S1743921323005276</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Modeling of the solar flare chromosphere and sub-THz radiation with FLARIX and RADYN

  • Original language description

    The origin of the sub-terahertz (sub-THz) component of radio emission from solar flares, which is characterized by the increase flux with frequency in the 100-400 GHz range, is considered. On the basis of equations of 1D non-LTE radiation hydrodynamics we simulated the altitude distribution of the plasma density and temperature inside the flare loop caused by the interaction of non-stationary beam of accelerated electrons in the form of a triangular pulse with the chromospheric plasma. The FLARIX numerical code was used to calculate the dynamics of the flare plasma parameters at different heights which are compared with the RADYN numerical code. We found that the characteristic heights of the formation of sub-THz emission vary over a wide range with time for both codes. The main contribution to the sub-THz emission comes from the chromospheric and transition region plasma with temperatures of 104 − 105 K.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • 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

  • Article name in the collection

    Proceedings of the International Astronomical Union

  • ISBN

  • ISSN

    1743-9213

  • e-ISSN

    1743-9221

  • Number of pages

    6

  • Pages from-to

    420-425

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Jerevan

  • Event date

    Aug 21, 2023

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article