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Time profile of type III bursts

✍ Scribed by T. Takakura; Y. Naito; K. Ohki


Publisher
Springer
Year
1975
Tongue
English
Weight
423 KB
Volume
41
Category
Article
ISSN
0038-0938

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Analysis of the time profile of type III
✍ A. Abrami; M. Messerotti; P. Zlobec; M. KarlickΓ½ πŸ“‚ Article πŸ“… 1990 πŸ› Springer 🌐 English βš– 343 KB

The time profile of two sets of isolated type III bursts, observed in the meter wavelength range at the Trieste Astronomical Observatory, was analyzed using a Fourier transform technique in order to accurately determine the decay constant of the exponential phase and to derive the exciter time profi

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✍ C. H. Barrow; A. Achong πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 303 KB

Solar type III bursts have been observed at fixed frequencies of 18, 22, 26 and 36 MHz during the period 1970-1974. 103 profiles have been al~alyzed in the manner introduced by Aubier and . Boischot (1972) whose results are generally confirmed. Average values for the exciter function duration were f

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✍ A. Achong; C. H. Barrow πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 468 KB

Observations of type III burst profiles at 18, 22, 26 and 36 MHz, by Barrow and Achong (1975), are used to calculate the form of the exciter function. The burst profile is treated as the convolution of an exciter function and an exponential decay function. The average form of the exciter profile is

Decay time of type III solar bursts obse
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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