We present the analysis of 64 type III solar bursts that drifted from 3.5 MHz down to the range 350-50 kHz between March 1968 and February 1970. Bursts arrival times were predicted by a simple model and then compared with observations. The results show that, as the bursts drift, the fundamental ofte
Heliographic longitude distribution of the flares associated with type III bursts observed at kilometric wavelengths
โ Scribed by Hector Alvarez; Fred T. Haddock; William H. Potter
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 370 KB
- Volume
- 31
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
We have grouped observed type III solar bursts according to the discrete frequencies of observation in the kilometrie wavelength range. For each group we have obtained the bursts' frequency of occurrence as a function of the heliographic longitude of the associated optical flares. We found that flares occurring east of a certain cutoff longitude do not produce bursts observable near the earth below a given frequency. The cutoff on the west is determined by observational limitation for flares beyond the limb. The mean longitude and the extreme eastern end of the longitude distribution both shift to the west as the radio frequency decreases. We interpret these findings in terms of radio wave propagation effects and curved trajectories of the bursts' exciter particles.
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