Radio emission from the magnetic equator of Uranus
Journal Article
·
· Journal of Geophysical Research; (USA)
- NASA Goddard Space Flight Center, Greenbelt, MD (USA)
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 plant at radial distances of approximately 2 to 3 R{sub v}. The most intense emission appears to be generated in association with the {var epsilon} ring at 2.0 R{sub v} radial distance. The authors infer a cold electron density of {le} 4 cm{sup {minus}3} in this region.
- OSTI ID:
- 5917876
- Journal Information:
- Journal of Geophysical Research; (USA), Vol. 94:A3; ISSN 0148-0227
- Country of Publication:
- United States
- Language:
- English
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