All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Numerical Simulation of Sub-Terahertz Emission of the Flare Chromosphere: the Event of July 4, 2012

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00552258" target="_blank" >RIV/67985815:_____/21:00552258 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1134/S0016793221070136" target="_blank" >https://doi.org/10.1134/S0016793221070136</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1134/S0016793221070136" target="_blank" >10.1134/S0016793221070136</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Numerical Simulation of Sub-Terahertz Emission of the Flare Chromosphere: the Event of July 4, 2012

  • Original language description

    The temporal evolution of thermal bremsstrahlung sub-THz emission from a flare chromosphere and transition region is analyzed based on the F-CHROMA solar flare model database (https://www.fchroma.org ) and solar flare observations with the RT-7.5 radio telescope at 93 and 140 GHz on July 4, 2012. The model is based on the RADYN numerical code, which describes the response of chromospheric background plasma to the action of a beam of accelerated electrons in the form of a triangular pulse. The positive slope of the spectrum in the sub-THz frequency range has been formed over the entire burst. A thin layer of low temperature and high plasma density (the so-called chromospheric condensation) appears. It moves to the region of higher altitudes and effectively absorbs the sub-THz emission. It is shown based on the RHESSI hard X-ray observations that the chromospheric thermal plasma cannot provide the observed sub-THz emission fluxes during the solar flare on July 4, 2012. The cause of the obtained discrepancy is discussed.

  • 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

    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

    2021

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Geomagnetism and Aeronomy

  • ISSN

    0016-7932

  • e-ISSN

    1555-645X

  • Volume of the periodical

    61

  • Issue of the periodical within the volume

    7

  • Country of publishing house

    RU - RUSSIAN FEDERATION

  • Number of pages

    7

  • Pages from-to

    1045-1051

  • UT code for WoS article

    000736717300020

  • EID of the result in the Scopus database

    2-s2.0-85122082341