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  • PST85

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DOI

The empirical model of disturbed magnetosphere of Tsyganenko and Usmanov (1982) and the semi-empirical model of the storm-time magnetospheric configuration of Tsyganenko (1981) are used to find the critical energy for non-adiabatic particle scattering in the midnight sector. Computed values of &, vs L are compared with the appropriate experimental data of Imhof et al. (1977). It is found that none of the considered models is able to reproduce the observed steep decrease of E,,,, with L. The steepest slope is given by the Tsyganenko model which includes a current sheet with the finite thickness. The current sheet thickness is a crucial parameter in the non-adiabatic scattering problem. In discussion we point to natural limitations of an empirical model as far as the current sheet thickness is to be determined. Imhof et al.‘s data as well as some magnetic field data sets seem to indicate that magnetosphere models incorporating a thin current sheet and allowing for the thickness dependence on the geocentric distance would probably be closer to reality than the considered models, at least during higher levels of magnetic activity.
Original languageEnglish
Pages (from-to)1433-1437
Number of pages5
JournalPlanetary and Space Science
Volume33
Issue number12
DOIs
StatePublished - Dec 1985

    Research areas

  • magnetosphere, particle scattering, pitch angle, magnetotail, current sheet

    Scopus subject areas

  • Physics and Astronomy(all)

ID: 27875027