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Observations of non-thermal radiation from planetsNonthermal radio emissions from earth, Jupiter, Saturn, and Uranus are reviewed. The dominant source of emission at each planet appears to be AKR-like auroral emission in the X-mode. O-mode emissions are substantially responsible. There is a remarkably constant scaling factor relating the total solar wind input power into each planetary system and the AKR-like auroral emissions.
Document ID
19900062861
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Kaiser, M. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Subject Category
Lunar And Planetary Exploration
Accession Number
90A49916
Distribution Limits
Public
Copyright
Other

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