Comparison of theory and in situ observations for electron and ion distributions in the near wake of the Explorer 31 and AE-C satellites

Details Comparison of theory and in situ observations for electron and ion distributions in the near wake of the Explorer 31 and AE-C satellites Comparison of theory and in situ observations for electron and ion distributions in the near wake of the Explorer 31 and AE-C satellites

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981p%26ss...29..975s&link_type=abstract

Planetary and Space Science, vol. 29, Sept. 1981, p. 975-987.

Computer Science

15

Ionospheric Electron Density, Ionospheric Ion Density, Near Wakes, Plasma Diagnostics, Plasma Potentials, Space Plasmas, Explorer 31 Satellite, Explorer 51 Satellite, Ion Currents, Plasma Currents, Poisson Equation, Rarefied Plasmas, Vlasov Equations

Scientific paper

Measurements of electron density, plasma potential, and mean ion mass from the Explorer 31 satellite, and measurements of ion current, plasma potential, and ion composition from the Atmosphere Explorer C satellite were used in a comparative study with Parker's theory regarding the charged particle distribution in the near wake of an ionospheric satellite (1976). It is shown that theory and experiment agree fairly well in the angle-of-attack range between 90 and 135 deg. In the maximum rarefaction zone (between 145 and 180 deg), however, the theoretical model overestimates the measured ion depletion by several orders of magnitude. A comparison between theory and the Explorer 31 electron measurements shows that the theory again overestimates the electron depletion. These discrepancies are mainly due to the use of a steady-state theory and a single ion equation (using a mean ion mass). Improved agreement between theory and experiment can be obtained by the use of the time-dependent Vlasov-Poisson equations with separate equations for the various ion species.

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