Association of type II solar radio bursts with coronal structures above H? filament channels
- 1 September 1984
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 94 (2) , 379-385
- https://doi.org/10.1007/bf00151325
Abstract
No abstract availableKeywords
This publication has 7 references indexed in Scilit:
- Correcting Low-Frequency Solar Radio Source Positions for Ionospheric RefractionPublications of the Astronomical Society of Australia, 1982
- The speeds of coronal mass ejection eventsSolar Physics, 1976
- Source heights of metre wavelength bursts of spectral types I and IIISolar Physics, 1976
- Dynamic response of an isothermal static corona to finite-amplitude disturbancesSolar Physics, 1975
- Behavior of the flare-produced coronal MHD wavefront and the occurrence of type II radio burstsSolar Physics, 1974
- Temperature-Density Structure in Coronal Helmets: the Quiescent Prominence and Coronal CavityThe Astrophysical Journal, 1972
- Solar BurstsAnnual Review of Astronomy and Astrophysics, 1963