Number of the records: 1  

Far-IR and Radio Thermal Continua in Solar Flares

  1. 1.
    SYSNO ASEP0334861
    Document TypeJ - Journal Article
    R&D Document TypeThe record was not marked in the RIV
    Subsidiary JOstatní články
    TitleFar-IR and Radio Thermal Continua in Solar Flares
    TitleDaleká infračervená a radiová kontinua ve slunečních erupcích
    Author(s) Kašparová, Jana (ASU-R) RID, ORCID
    Heinzel, Petr (ASU-R) RID, ORCID
    Karlický, Marian (ASU-R) RID, ORCID
    Moravec, Z. (CZ)
    Varady, M. (CZ)
    Source TitleCentral European Astrophysical Bulletin - ISSN 1845-8319
    Roč. 33, - (2009), s. 309-315
    Number of pages7 s.
    Languageeng - English
    CountryHR - Croatia
    Keywordssolar flares ; radiative hydrodynamics ; continuum emission
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGA205/04/0358 GA ČR - Czech Science Foundation (CSF)
    GP205/06/P135 GA ČR - Czech Science Foundation (CSF)
    GA205/07/1100 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    AnnotationWith the invention of new far-infrared (FIR) and radio mm and sub-mm instruments (DESIR on SMESE satellite, ESO-ALMA), there is a growing interest in observations and analysis of solar flares in this so far unexplored wavelength region. Two principal radiation mechanisms play a role: the synchrotron emission due to accelerated particle beams moving in the magnetic field and the thermal emission due to the energy deposit in the lower atmospheric layers. In this contribution we explore the time-dependent effects of beams on thermal FIR and radio continua. We show how and where these continua are formed in the presence of time dependent beam heating and non-thermal excitation/ionisation of the chromospheric hydrogen plasma.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2010
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.