Published September 30, 1981
| Version v1
Journal article
Jovian S burst sources
Creators
- 1. Observatoire de Paris, Section d'Astrophysique de Meudon, 92190 Meudon, France
Description
By using the high resolution observation of Nancay observatory, we have been able to identify the S burst emission on the planetary radio astronomy (PRA) records of Voyager. It is shown that the S bursts occur in two regions of the Phi10-CML plane (S-IoB and S-IoA'C regions). In these regions the S burst emission is arranged into a pattern of repetitive features, drifting negatively. These features could be incomplete vertex late arcs. We show that the S burst pattern is distinct from the pattern of the Io-controlled emission. These results are discussed in the frame of Goldstein and Thieman's arc model
Additional details
Publishing Information
- Journal Title
- J. Geophys. Res.
- Journal Volume
- 86
- Journal Issue
- A10
- Series
- J. Geophys. Res.
- Journal Page Range
- 8564-8568
- ISSN
- 0022-1406
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 13676738
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- EMISSION SPECTRA; JUPITER PLANET; LONG WAVE RADIATION; PLANETARY MAGNETOSPHERES; SATELLITES; WAVE PROPAGATION
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; PLANETARY ATMOSPHERES; PLANETS; RADIATIONS; RADIOWAVE RADIATION; SPECTRA