Type llI bursts were observed between 3.5 MHz and 50 kHz by the University of Michigan radio astronomy experiment aboard the OGO-5 satellite. Decay times were measured and then combined with published data ranging up to about 200 MHz. The observed decay times increase with decreasing frequency but
The prevalence of second harmonic radiation in type III bursts observed at kilometric wavelengths
โ Scribed by F. T. Haddock; Hector Alvarez
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 696 KB
- Volume
- 29
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
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 often disappears below a certain frequency range while the second harmonic remains. Below about 1 MHz the second harmonic occurrence predominates, Recognizing this fact we deduce a mean velocity of 0.32c โข for the exciter particles, where the uncertainty is the standard error and c the velocity of light in vacuum; the electron density model used is comparable to a solar wind model.
๐ SIMILAR VOLUMES
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 flar
Using the data from our experiments on the IMP-6 (Explorer 43) satellite, we have examined over 200 type III bursts at kilometric wavelengths, including 16 bursts which were accompanied by >18 keV electron events with sharp onsets, in a search for the electrostatic waves which, according to theory,