Offset, tilted dipole models of Uranian smooth high-frequency radio emission

Details Offset, tilted dipole models of Uranian smooth high-frequency radio emission Offset, tilted dipole models of Uranian smooth high-frequency radio emission

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....9514977s&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, Sept. 1, 1990, p. 14977-14986.

Astronomy and Astrophysics

Astronomy

4

Dipoles, Radio Emission, Uranus (Planet), Voyager 2 Spacecraft, Computerized Simulation, High Frequencies, Miranda, Planetary Magnetospheres, Radio Astronomy

Scientific paper

The smooth high-frequency (SHF) component of the radio emission detected during the Voyager 2 encounter with Uranus (January 1986) is studied. An offset tilted dipole (OTD) investigation of the SHF emission at L shells is carried out within the range of the bursty source locations. A viable high L shell model is presented. It is suggested that Miranda, which reaches a minimum L shell at L = 5, may be related to the timing of several types of radio emissions.

Affiliated with

Also associated with

No associations

Rating

Offset, tilted dipole models of Uranian smooth high-frequency 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 Offset, tilted dipole models of Uranian smooth high-frequency radio emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Offset, tilted dipole models of Uranian smooth high-frequency radio emission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1404942