Properties of metre-wavelength solar bursts associated with coronal mass ejections
- 1 May 1986
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 105 (1) , 149-171
- https://doi.org/10.1007/bf00156384
Abstract
No abstract availableKeywords
This publication has 25 references indexed in Scilit:
- A positional comparison between coronal mass ejection events and solar type II burstsSolar Physics, 1985
- Associations between coronal mass ejections and metric type II burstsThe Astrophysical Journal, 1984
- Associations between coronal mass ejections and soft X-ray eventsThe Astrophysical Journal, 1983
- Association between gradual hard X-Ray emission and metric continua during large flaresSolar Physics, 1983
- Solar type II radio emission and the shock drift acceleration of electronsThe Astrophysical Journal, 1983
- Electron acceleration and radiation signatures in loop coronal transientsThe Astrophysical Journal, 1982
- Origin and Location of the Hard X-Ray Emission in a Two-Ribbon FlareThe Astrophysical Journal, 1981
- Prompt solar proton events and coronal mass ejectionsSolar Physics, 1978
- A Study of Solar Flare Continuum Events Observed at Metre WavelengthsAustralian Journal of Physics, 1978
- The morphological and statistical properties of solar X-ray events with long decay timesThe Astrophysical Journal, 1977