Computer Science
Scientific paper
Oct 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980natur.287..815d&link_type=abstract
Nature, vol. 287, Oct. 30, 1980, p. 815-817.
Computer Science
1
Io, Jupiter Atmosphere, Planetary Radiation, Radio Emission, Flux (Rate), Ground Stations, Low Frequencies, Satellite Observation, Jupiter, Radio Emissions, Satellites, Io, Decameter Waves, Intensity, Wavelengths, Frequencies, Voyager 1, Rae 1, Comparisons, Observations, Data, Source Medium
Scientific paper
The possibility of Io controlling Jovian decametric radio emission, particularly in the region below 22 MHz, is discussed. Results of a two-year survey at 26.3 at 26.3 MHz are presented which demonstrate the control of Io over a high-intensity storm component of the radio emission and the independence of a weak radio component from the phase of Io, as was observed at lower frequencies. It is thus hypothesized that Io control is a flux-dependent rather than a frequency-dependent phenomenon, and results of analyses at 18 and 10 MHz which support this hypothesis are presented. The apparent correlation between frequency and Io control is thus shown to result from a selection effect due to the increase of non-Io emission with decreasing frequency and relative antenna detection threshold. This result implies a contiguous Io-controlled source region extending out several Jovian radii along the Io flux tube.
No associations
LandOfFree
Io control of Jovian radio emission 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 Io control of Jovian radio emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Io control of Jovian radio emission will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-949809