Published December 1, 1980
| Version v1
Journal article
Some spectral characteristics of the hectometric Jovian emission
Creators
- 1. Observatoire de Paris, Section D'Astrophysique, 92-Meudon (Hauts de Seine), France
Description
The study of the dynamic spectra of hectometric Jovian emission (f<1.3 MHz) for the period January to June 1978 from the planetary radio astronomy (PRA) experiment on the Voyager 1 and 2 spacecraft shows that its shape is stable with the rotation of the planet. However, there are noticeable differences between the spectra observed at one-month intervals by one spacecraft, or simultaneously by the two spacecraft, which can be clearly related neither to an effect of Io nor the the Jovicentric decination of the observer
Additional details
Publishing Information
- Journal Title
- J. Geophys. Res.
- Journal Volume
- 85
- Journal Issue
- A12
- Series
- J. Geophys. Res.
- Journal Page Range
- 6877-6882
- ISSN
- 0022-1406
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 12597990
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- JUPITER PLANET; PLANETARY MAGNETOSPHERES; RADIOWAVE RADIATION; ROTATION; SPECTRAL DENSITY; VARIATIONS; VOYAGER SPACE PROBES
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; FUNCTIONS; PLANETARY ATMOSPHERES; PLANETS; RADIATIONS; SPACE VEHICLES; SPECTRAL FUNCTIONS