Number of the records: 1  

Shock-drift accelerated electrons and n-distribution

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    SYSNO ASEP0463131
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleShock-drift accelerated electrons and n-distribution
    Author(s) Vandas, Marek (ASU-R) RID, ORCID
    Karlický, Marian (ASU-R) RID, ORCID
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 591, July (2016), A127/1-A127/6
    Number of pages6 s.
    Publication formOnline - E
    Languageeng - English
    CountryFR - France
    Keywordsshock waves ; acceleration of particles ; Sun flares
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    R&D ProjectsGA14-19376S GA ČR - Czech Science Foundation (CSF)
    GA15-17490S GA ČR - Czech Science Foundation (CSF)
    GAP209/12/0103 GA ČR - Czech Science Foundation (CSF)
    Institutional supportASU-R - RVO:67985815
    UT WOS000379141300136
    EID SCOPUS84977110680
    DOI10.1051/0004-6361/201527183
    AnnotationBy analyzing soft X-ray spectra observed during the impulsive phase of several solar flares, the n-distribution function of superthermal electrons has been detected. In the paper we try to answer the question of whether electrons with this type of distribution function can be produced in a shock, e.g. in a flare termination shock. We use analytical and numerical methods to compute distribution functions of electrons accelerated by a shock. We analytically derive the distribution functions of reflected electrons at quasi-perpendicular shocks. We also consider the influence of the electrostatic cross-shock potential, shock curvature, and the role of the upstream seed population on these distributions. The computed distributions are compared with the n-distributions. We found that a high-energy part of the distribution of electrons reflected at a quasi-perpendicular shock can be very well fitted by the n-distribution in all the cases we studied. This provides a chance to detect the flare termination shock.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2017
Number of the records: 1  

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