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- W2035157962 abstract "view Abstract Citations (14) References (17) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS An Upper Limit to X-Ray Emission from Saturn Gilman, D. A. ; Hurley, K. C. ; Seward, F. D. ; Schnopper, H. W. ; Sullivan, J. D. ; Metzger, A. E. Abstract X-rays are produced in auroral discharges, and their measurement can serve to characterize the interaction processes responsible for the aurora itself. The existence of auroral activity on Saturn was suggested by the observation of a magnetosphere by Pioneer 11 and confirmed by UV measurements during the Voyager encounters. The detection of X-rays from Jupiter with the Einstein Observatory (HEAO 2) satellite provided the impetus for a subsequent observation of Saturn. No emission was detected. This article presents the upper limit established by the observation and derives an expected emission level assuming X-ray production to be the result of bremsstrahlung from keV electrons precipitating into Saturn's atmosphere. The difference is a factor of 100. Publication: The Astrophysical Journal Pub Date: January 1986 DOI: 10.1086/163820 Bibcode: 1986ApJ...300..453G Keywords: Auroral Arcs; Heao 2; Planetary Radiation; Saturn (Planet); Saturn Atmosphere; X Ray Sources; Bremsstrahlung; Energy Transfer; Pioneer 11 Space Probe; Planetary Magnetospheres; Ultraviolet Astronomy; X Ray Spectra; SATURN; X-RAYS; EMISSIONS; MAGNETOSPHERE; PIONEER 11; ULTRAVIOLET; WAVELENGTHS; VOYAGER MISSIONS; SPACECRAFT OBSERVATIONS; SOURCE; Lunar and Planetary Exploration; Saturn; PLANETS: SATURN; X-RAYS: SOURCES full text sources ADS |" @default.
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- W2035157962 date "1986-01-01" @default.
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- W2035157962 title "An upper limit to X-ray emission from Saturn" @default.
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