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- W2096553764 abstract "The spatial and temporal variations of the thermal plasma between L = 2 and L = 4 over the altitude range 3000 to 5700 km have been studied. The data were obtained from two spherical electrostatic analyzers flown on the polar orbiting satellite OV 3–1 between April 1966 and February 1967. During magnetically quiet periods the ionization density is characteristically found to decrease monotonically with increasing L. Between L = 2 and L = 3 a dependence of the average electron density on longitude is found, with the maximum between April and August occurring at 150°E and the minimum at 300°E. At L < 4, major charge density irregularities are found on 30% of the orbits at times of quiet to moderate magnetic activity, sometimes consisting of over an order of magnitude changes in density in less than 0.1 L. Comparison of density profiles obtained on the same day at different longitudes shows the irregularities to be of limited longitudinal extent. It is suggested that the depletions result from inward shifts of sectors of the plasmapause to lower L shells by E × B drifts. Large-amplitude, small-scale irregularities extending over tens of kilometers are often superimposed on the major density gradients and appear to be the result of plasma instabilities." @default.
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- W2096553764 date "1972-09-01" @default.
- W2096553764 modified "2023-09-26" @default.
- W2096553764 title "Spatial and temporal variations of the thermal plasma between 3000 and 5700 kilometers atL= 2 to 4" @default.
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- W2096553764 doi "https://doi.org/10.1029/ja077i025p04734" @default.
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