Astronomy and Astrophysics – Astronomy
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980georl...7..389k&link_type=abstract
Geophysical Research Letters, vol. 7, May 1980, p. 389-392.
Astronomy and Astrophysics
Astronomy
26
Emission Spectra, Jupiter (Planet), Planetary Radiation, Radio Astronomy, Radio Spectra, Spectral Line Width, Io, Planetary Rotation, Plasma Waves, Polarization (Waves), Voyager 1 Spacecraft, Voyager 2 Spacecraft, Wave Propagation, Waveforms, Jupiter, Radiation, Kilometer Waves, Radio Spectra, Bandwidths, Emissions, Polarization, Observations, Data, Voyager 1, Flux, Density, Frequency, Rotation, Plasmas, Torus, Spectrum, Pra, Plasma Wave Instrument
Scientific paper
The paper describes a new component of Jupiter's radio spectrum. This component emits in a very narrow bandwidth (less than 40 kHz) near 100 kHz. Its waveform is a very smooth and gradual rise and subsequent fall in intensity over typically two hours. The emission is polarized with left-hand polarization associated with the Jovian northern magnetic hemisphere and righthand with the south. The most interesting feature of the emission is its deviation from a strict System III rotation period repetition rate. The emission source of this narrow-band component clearly rotates slower by 3-5% than all other forms of Jovian radio emission. Propagation considerations coupled with this observed lack of corotation point to a source region near the magnetic equatorial plane at the outer 'edge' of the Io plasma torus.
Desch Michael D.
Kaiser Michael L.
No associations
LandOfFree
Narrow-band Jovian kilometric radiation - A new radio component does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Narrow-band Jovian kilometric radiation - A new radio component, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Narrow-band Jovian kilometric radiation - A new radio component will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1359490