Spectra of complex Jovian S-storms can be interpreted as groups of tilted-V variants. In such an approach the basic components (wide-range S-bursts, narrow-range S-trains, emissions of type N, and shadow events) are arranged in a predictable sequence. It seems that the application of tilted-V varian
Bursts of type N in Jupiter's decametric radio spectra
β Scribed by Jorma J. Riihimaa
- Publisher
- Springer Netherlands
- Year
- 1985
- Tongue
- English
- Weight
- 582 KB
- Volume
- 32
- Category
- Article
- ISSN
- 1573-0794
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β¦ Synopsis
Dynamic spectra of Jupiter's decamctric emission often display narrow-band features, referred to as events of type N (Carr et al., 1983). The average bandwidth of these emissions is in the vicinity of 200 kHz, their durations are typically in the decasecond range, and thcirj-t slopes arc small and random. Although the N-bursts can be described as narrow-band L-bursts, it seems that they are rcalkd to S-bursts in their area ol' occurrence in the IO-B region, the durations of the emission envelopes, and their bandwidths. Possible implications are discussed.
π SIMILAR VOLUMES
The paper describes the polarization characteristics of decametric type III solar radio bursts at two closely spaced frequencies, 34.993 and 34.997 MHz. From the simultaneous orientation angle measurements at these two frequencies, it is concluded that the total Faraday rotation suffered by type Ill