Radio emission from the magnetic equator of Uranus

Details Radio emission from the magnetic equator of Uranus Radio emission from the magnetic equator of Uranus

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94.2399k&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 94, March 1, 1989, p. 2399-2404.

Physics

11

Magnetic Equator, Planetary Radiation, Radio Emission, Uranus (Planet), Narrowband, Planetary Magnetic Fields, Polarization Characteristics, Radiation Sources, Voyager 2 Spacecraft, Uranus, Radio Emissions, Magnetic Properties, Source, Equatorial Regions, Epsilon Ring, Voyager 2 Mission, Spacecraft Observations, Pra Instrument, Diagrams, Position (Location), Intensity, Polarization, Comparisons, Electrons, Density

Scientific paper

The major observational characteristics of the smooth, narrow bandwidth component of Uranus' radio emissions are well described by sources radiating near the local electron gyrofrequency, confined to the magnetic equatorial plane and encircling the planet at radial distances of approximately 2 to 3 R(U). The most intense emission appears to be generated in association with the epsilon ring at 2.0 R(U) radial distance. A cold electron density of less than or equal to 4/cu cm are inferred in this region.

Affiliated with

Also associated with

No associations

Rating

Radio emission from the magnetic equator of Uranus 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 Radio emission from the magnetic equator of Uranus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio emission from the magnetic equator of Uranus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1804373