Electron acceleration in flares inferred from radio and hard X-ray emissions
- 1 March 1986
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 104 (1) , 179-185
- https://doi.org/10.1007/bf00159960
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Solar flare development during the impulsive phase as deduced from correlated radio and hard X-ray observationsThe Astrophysical Journal, 1985
- Simultaneous microwave observations of solar flares at 6 and 20 cm wavelengths using the VLASolar Physics, 1985
- Coronal X-ray activity preceding solar flaresSolar Physics, 1985
- Correlation of solar decimetric radio bursts with X-ray flaresSolar Physics, 1985
- Radio spikes and the fragmentation of flare energy releaseSolar Physics, 1985
- A study of flare buildup from simultaneous observations in microwave, H-alpha, and UV wavelengthsThe Astrophysical Journal Supplement Series, 1985
- Decimetric type III radio bursts and associated hard X-ray spikesSolar Physics, 1984
- The computer-controlled solar radio spectrometer ?IKARUS?Solar Physics, 1982
- Spatial structure of greater than 100 keV X-ray sources in solar flaresThe Astrophysical Journal, 1982
- Energetic electrons, Type III radio bursts, and impulsive solar flare X-raysThe Astrophysical Journal, 1981