Computer Science
Scientific paper
Nov 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991iowa.rept.....c&link_type=abstract
Final Report, 15 Aug. 1987 - 30 Sep. 1991 Iowa Univ., Iowa City.
Computer Science
Neptune (Planet), Planetary Radiation, Radio Emission, Uranus (Planet), Auroras, Planetary Rotation, Plasmasphere, Space Plasmas, Spectrograms, Superhigh Frequencies
Scientific paper
Progress under this grant has included identifying certain new radio emission components and determining the source location of both these and the two major Uranian radio emission (the SHF and bursty components) by a unique new statistical minimization technique. This new source location technique has subsequently also been applied at Neptune, with considerable success. New radio spectrograms have been prepared to clarify the behavior of such emissions, using both the usual 48-second, log-averaged data and the original 6-second PRA data, the latter showing a number of interesting new features. Also, a plasmasphere was discovered at Uranus, auroral plasma cavities were discovered at both Uranus and Neptune, and it was found that the currently-accepted rotation period for Uranus is in error by a small amount.
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