Motion of Jupiter's decametric sources in Io phase

Details Motion of Jupiter's decametric sources in Io phase Motion of Jupiter's decametric sources in Io phase

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apl....16...83t&link_type=abstract

Astrophysical Letters, vol. 16, no. 3, 1975, p. 83-86.

Mathematics

Probability

3

Decametric Waves, Io, Jupiter (Planet), Planetary Radiation, Radio Emission, High Resolution, Histograms, Oscillations, Secular Variations

Scientific paper

Decametric radio observations of Jupiter by the Universities of Florida, Chile, and Texas have been combined to achieve 2-deg resolution in histograms of occurrence probability vs Io phase for the years 1957 through 1972. Under this high resolution, the centroids and maxima of the Io-related source A, B, and C peaks appear to oscillate sinusoidally with a time scale of the order of a decade, mirroring the drift of source A in central-meridian-longitude coordinates. The Io-related peaks are persistently asymmetric, being skewed toward earlier positions of Io, and the primary peaks are often preceded by smaller secondary peaks.

Affiliated with

Also associated with

No associations

Rating

Motion of Jupiter's decametric sources in Io phase 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 Motion of Jupiter's decametric sources in Io phase, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Motion of Jupiter's decametric sources in Io phase will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-998935