0124595 - ASU-R 20000051 RIV DE eng J - Článek v odborném periodiku
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
Grant CEP: GA AV ČR IAA3003707
Výzkumný záměr: CEZ:AV0Z1003909
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 1.630, rok: 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.
Trvalý link: http://hdl.handle.net/11104/0022854