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Title: Variation of the plasma-sheet polytropic index along the midnight meridian in a finite-width magnetotail. Technical report

Abstract

The polytropic index is obtained as a function of distance along the midnight meridian in the terrestrial magnetotail. As our purpose is to establish the effects of the finite width of the magnetotail, we use a simple theoretical model of plasma sheet convection, i.e., two-dimensional field structure and adiabatic inward convection of a uniform distant tail source. Particle orbits are treated independently for portions of the phase space distribution on shells of constant energy. On the midnight meridian, the moments of the distribution are parameterized by tau, the ratio of half the cross-tail potential energy to the characteristic Maxwellian energy of a distant down-tail plasma source. We infer from the model the plasma pressure, P, and the number density, n, along the midnight meridian as a function of tau. P and n define locally an effective polytropic index. Gamma ranges between 5/3 and 1, depending on the value of tau and on geocentric distance. The qualitative differences between the recent empirical determinations of the polytropic index by Baumjohann and Paschmann and Huang et al. may be accounted for in part by this simple model.

Authors:
;
Publication Date:
Research Org.:
Aerospace Corp., El Segundo, CA (USA). Laboratory Operations
OSTI Identifier:
6046665
Report Number(s):
AD-A-225948/9/XAB; TR-0089(4940-06)-8
CNN: F04701-88-C-0089
Resource Type:
Technical Report
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; PLASMA SHEET; CONVECTION; MATHEMATICAL MODELS; CHARGE DENSITY; DISTANCE; EARTH MAGNETOSPHERE; MAGNETOTAIL; MAXWELL EQUATIONS; PLASMA; PROGRESS REPORT; RADIATION PRESSURE; SIZE; DIFFERENTIAL EQUATIONS; DOCUMENT TYPES; EARTH ATMOSPHERE; ENERGY TRANSFER; EQUATIONS; HEAT TRANSFER; MASS TRANSFER; PARTIAL DIFFERENTIAL EQUATIONS; 640201* - Atmospheric Physics- Auroral, Ionospheric, & Magetospheric Phenomena

Citation Formats

Spence, H E, and Kivelson, M G. Variation of the plasma-sheet polytropic index along the midnight meridian in a finite-width magnetotail. Technical report. United States: N. p., 1990. Web.
Spence, H E, & Kivelson, M G. Variation of the plasma-sheet polytropic index along the midnight meridian in a finite-width magnetotail. Technical report. United States.
Spence, H E, and Kivelson, M G. 1990. "Variation of the plasma-sheet polytropic index along the midnight meridian in a finite-width magnetotail. Technical report". United States.
@article{osti_6046665,
title = {Variation of the plasma-sheet polytropic index along the midnight meridian in a finite-width magnetotail. Technical report},
author = {Spence, H E and Kivelson, M G},
abstractNote = {The polytropic index is obtained as a function of distance along the midnight meridian in the terrestrial magnetotail. As our purpose is to establish the effects of the finite width of the magnetotail, we use a simple theoretical model of plasma sheet convection, i.e., two-dimensional field structure and adiabatic inward convection of a uniform distant tail source. Particle orbits are treated independently for portions of the phase space distribution on shells of constant energy. On the midnight meridian, the moments of the distribution are parameterized by tau, the ratio of half the cross-tail potential energy to the characteristic Maxwellian energy of a distant down-tail plasma source. We infer from the model the plasma pressure, P, and the number density, n, along the midnight meridian as a function of tau. P and n define locally an effective polytropic index. Gamma ranges between 5/3 and 1, depending on the value of tau and on geocentric distance. The qualitative differences between the recent empirical determinations of the polytropic index by Baumjohann and Paschmann and Huang et al. may be accounted for in part by this simple model.},
doi = {},
url = {https://www.osti.gov/biblio/6046665}, journal = {},
number = ,
volume = ,
place = {United States},
year = {1990},
month = {8}
}

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