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  • 1
    Publication Date: 2011-08-24
    Description: A method is presented for analytically representing the magnetic field due to the cross-tail current and its closure on the magnetopause. It is an extension of a method used by Tsyganenko (1989b) to confine the dipole field inside an ellipsoidal magnetopause using a scalar potential. Given a model of the cross-tail current, the implied net magnetic field is obtained by adding to the cross-tail current field a potential field B = - del gamma, which makes all field lines divide into two disjoint groups, separated by the magnetopause (i.e., the combined field is made to have zero normal component with the magnetopause). The magnetopause is assumed to be an ellipsoid of revolution (a prolate spheroid) as an approximation to observations (Sibeck et al., 1991). This assumption permits the potential gamma to be expressed in spheroidal coordinates, expanded in spheroidal harmonics and its terms evaluated by performing inversion integrals. Finally, the field outside the magnetopause is replaced by zero, resulting in a consistent current closure along the magnetopause. This procedure can also be used to confine the modeled field of any other interior magnetic source, though the model current must always flow in closed circuits. The method is demonstrated on the T87 cross-tail current, examples illustrate the effect of changing the size and shape of the prescribed magnetopause and a comparison is made to an independent numerical scheme based on the Biot-Savart equation.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research (ISSN 0148-0227); 99; A10; p. 19,393-19,402
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  • 2
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    In:  CASI
    Publication Date: 2005-11-30
    Description: Theoretical work designed to bridge the gap between celestial mechanics and the motion of charged particles in magnetic fields is presented. Attempts are made to devise a simple uninvolved method to solve adiabatic invariant motion problems. The method is illustrated by solving a problem involving the motion of a slowly perturbed harmonic oscillator.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 71-74
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  • 3
    Publication Date: 2006-10-26
    Description: Low frequency power spectrum of cosmic ray variations during igy
    Keywords: FLUID MECHANICS
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  • 4
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    In:  Other Sources
    Publication Date: 2011-08-16
    Description: International geomagnetic reference field 1965 geomagnetic potential rate of change and transformation to dipole coordinates
    Keywords: GEOPHYSICS
    Type: ; YAL SOCIETY (
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  • 5
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    Publication Date: 2011-08-16
    Description: Canonical perturbation theory formulation applied to Poincare-von Zeipel method
    Keywords: SPACE SCIENCES
    Type: ; 99-102 (
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  • 6
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    In:  Other Sources
    Publication Date: 2011-08-16
    Description: Drift shells of trapped particles starting from a single field line in the earth's magnetic field may become separated owing to an electric field. By using the formalism of the shell-splitting function, this separation is calculated for an arbitrary curl-free time-independent electric field satisfying E.B = 0, with no limitation on the particle's longitudinal excursion. The effect of nondipole field components is also taken into account to the lowest order.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 76; Nov. 1
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  • 7
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    In:  Other Sources
    Publication Date: 2011-08-16
    Description: Recently, Svalgaard and Heppner reported two separate features of the polar electromagnetic field that correlate with the dawn-dusk component of the interplanetary magnetic field. This work attempts to explain these findings in terms of properties of the open magnetosphere. The topology and qualitative properties of the open magnetosphere are first studied by means of a simple model, consisting of a dipole in a constant field. Many such properties are found to depend on the separation line, a curve connecting neutral points and separating different field line regimes. In the simple model it turns out that the electric field in the central polar cap tends to point from dawn to dusk for a wide variety of external fields, but, near the boundary of the polar cap, electric equipotentials are deformed into crescents.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 78; Nov. 1
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  • 8
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    In:  Other Sources
    Publication Date: 2011-08-10
    Description: Calculation of magnetic shell parameters based on Pennington perturbation method
    Keywords: GEOPHYSICS
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  • 9
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    In:  Other Sources
    Publication Date: 2011-08-11
    Description: Motion of magnetic lines of force including analysis of fluids with finite high conductivity
    Keywords: PHYSICS, GENERAL
    Type: SPACE SCIENCE REVIEWS
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  • 10
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    Publication Date: 2011-08-12
    Description: Euler potentials and geomagnetic drift shells, discussing charged particle motion in magnetic field
    Keywords: GEOPHYSICS
    Type: ; ADEMIE DES SCIENCES
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