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Chromospheric evaporation shock and reduced optical thickness drifting in the 1-4.5 GHz range

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    0124595 - ASU-R 20000051 RIV DE eng J - Journal Article
    Karlický, Marian
    Chromospheric evaporation shock and reduced optical thickness drifting in the 1-4.5 GHz range.
    Astronomy & Astrophysics. Roč. 338, č. 3 (1998), s. 1084-1088. ISSN 0004-6361. E-ISSN 1432-0746
    R&D Projects: GA AV ČR IAA3003707
    Institutional research plan: CEZ:AV0Z1003909
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 1.630, year: 1998

    Using a 1-D numerical hydrodynamic model, the evaporation shock evolution is computed in the solar atmosphere having the density profile derived from radioastronomical observations. Then the optical thickness of the 1-4,5 GHz plasma emission on harmonic frequency is computed.
    Permanent Link: http://hdl.handle.net/11104/0022854


     
     

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