Energy interconnection between the plasma cloud ejected from the active region and the shock wave
- 1 May 1986
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 105 (1) , 101-109
- https://doi.org/10.1007/bf00156380
Abstract
No abstract availableKeywords
This publication has 30 references indexed in Scilit:
- Radio data and a theoretical model for the fast-mode MHD shock wave generated by the solar flare of 1973 September 5, 18:26 UTThe Astrophysical Journal, 1979
- The large coronal transient of 10 June 1973Solar Physics, 1975
- Correlation of a flare-wave and type II burstSolar Physics, 1974
- The flares of July 6 and 8, 1968Solar Physics, 1970
- Expanding arch structure of a solar radio outburstSolar Physics, 1970
- Position Measurements of a Harmonic Type II Solar BurstPublications of the Astronomical Society of Australia, 1969
- Radio Evidence for the Propagation of Magnetohydrodynamic Waves along Curved Paths in the Solar CoronaPublications of the Astronomical Society of Australia, 1969
- Evidence of Type II and Moving Type IV Solar Bursts Excited by a Common Shock WavePublications of the Astronomical Society of Australia, 1969
- Metre-wave Dynamic Spectrum of a Solar Flare on 9 June 1968Publications of the Astronomical Society of Australia, 1968
- Type II Solar Radio Bursts Observed with the Culgoora Radioheliograph during a Flare on 17 June 1968Publications of the Astronomical Society of Australia, 1968