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Chromospheric evaporation shock and reduced optical thickness drifting in the 1-4.5 GHz range
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SYSNO ASEP 0124595 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Ostatní články Title Chromospheric evaporation shock and reduced optical thickness drifting in the 1-4.5 GHz range Author(s) Karlický, Marian (ASU-R) RID, ORCID Source Title Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 338, č. 3 (1998), s. 1084-1088Number of pages 5 s. Language eng - English Country DE - Germany Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects IAA3003707 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z1003909 - ASU-R Annotation 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. Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2001
Number of the records: 1