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In ecliptic observations of Jovian radio emissions by Ulysses - Comparison with Voyager resultsDuring the Ulysses inbound cruise to Jupiter the Unified Radio and Plasma Wave (URAP) experiment observed a variety of the planet's radio components in the frequency range below 1 MHz. Most of these emissions were already detected by the Voyager Radio Astronomy and Plasma Wave experiments, however, with much less sensitivity and different spectral coverage. These different radio components within the URAP dynamic spectra are identified, and their appearance with the previous Voyager observations are compared.
Document ID
19920064828
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lecacheux, A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Pedersen, B. M.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Zarka, PH.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Aubier, M. G.
(Paris Observatoire, Meudon, France)
Desch, M. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Farrell, W. M.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kaiser, M. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Macdowall, R. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Stone, R. G.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 15, 2013
Publication Date
June 19, 1992
Publication Information
Publication: Geophysical Research Letters
Volume: 19
Issue: 12, J
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Accession Number
92A47452
Distribution Limits
Public
Copyright
Other

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