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  • 1
    Publication Date: 2019-06-27
    Description: Features in the equatorial zone of Jupiter show that the equatorial plume reported by Pioneer 10 has existed for an 11-year interval. During this interval the plume has shown an acceleration which can be interpreted as a constant component of 3 x 10 to minus 8th power m/sq cm and a sinusoidal component which anticorrelates with the planetocentric declination of the sun, D sub s, and has an amplitude of -0.96 meters per second per degree change of D sub s. The sinusoidal component has been interpreted in terms of solar heating. Throughout this interval of time the equatorial zone has appeared abnormally dark and has contained many dark projections along the northern edge. When the plume approaches to within 25 to 30 deg of these features they are deflected in the direction of motion of the plume and then dissipate or become obscured as the plume passes. After passage of the plume normal features are again observed.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-CR-142894 , TN-75-48
    Format: application/pdf
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  • 2
    Publication Date: 2019-06-27
    Description: Recent longitudinal measurements of Jupiter's Red Spot are presented to illustrate the constancy of the 90-day oscillation. Observational parameters of the Red Spot, the three south temperate ovals, and a summary of the zenographic latitudes of the belts are tabulated for the time interval from 1972 to 1975. Drift rates and the mean latitudes of the atmospheric currents for the 1974-75 apparition are presented.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Contrib. of the Observatory of N. Mex. State Univ., Vol. 1, No. 4; p 176-190
    Format: text
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  • 3
    Publication Date: 2019-06-27
    Description: Analysis of features in the Equatorial Zone of Jupiter has shown that the equatorial plume reported by Pioneer 10 has existed for an 11-yr interval. During this interval, the plume has shown an acceleration which can be interpreted as a constant component of 3 hundred-millionths m/sec-squared and a sinusoidal component which anticorrelates with the planetocentric declination of the sun and has an amplitude of -0.96 m/sec per degree change of planetocentric declination. The sinusoidal component has been interpreted in terms of solar heating. Throughout this interval of time, the Equatorial Zone has appeared abnormally dark and has contained many dark projections along the northern edge. When the plume approaches to within 25 to 30 deg of these features, they are deflected in the direction of motion of the plume and then dissipate or become obscured as the plume passes. After passage of the plume, normal features are again observed.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Format: text
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