Alfven waves from an electrodynamic tethered satellite system
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
The operation of an electrodynamic tethered satellite system in the ionosphere in a steady state (constant current) mode is intimately connected with the elctromagnetic plasma waves the system excites, since these waves carry the electrical currents that complete the tethered system/plasma circuit. The analysis reported here determines (within cold plasma theory) the ionospheric currents and associated wave impedance based on a tethered system current distribution that takes into account the dumbbell geometry of the system. The analysis is not restricted to terminating satellite dimensions that are much greater than the systems velocity divided by the ion cyclotron frequency, as has been the case in almost all previous studies of the problem. When this is not satisfied, the Alfven wings (field line sheet currents) are found to be wider than the dimensions of the terminating satellite, a result of the wave nature of the phenomenon and restrictions on perpendicular wavelengths along the line-of-flight direction. Previously reported large wave impedances associated with an orbiting wire, which would limit tether currents to low values, are shown to be inapplicable to a more realistic model of the tethered system. The calculated wave impedance, which depends weakly on the system dimensions, is only a few ohms or less in low Earth orbit.
- OSTI ID:
- 6050478
- Journal Information:
- Journal of Geophysical Research; (United States), Vol. 93:A2; ISSN 0148-0227
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
GENERAL PHYSICS
IONOSPHERE
SATELLITES
ELECTRODYNAMICS
ALFVEN WAVES
CHARGE COLLECTION
ELECTRIC CABLES
ELECTRIC CURRENTS
ELECTRICAL INSULATION
GEOMAGNETIC FIELD
GEOMETRY
MOTION
PLASMA WAVES
CABLES
CONDUCTOR DEVICES
CURRENTS
EARTH ATMOSPHERE
ELECTRICAL EQUIPMENT
EQUIPMENT
HYDROMAGNETIC WAVES
MAGNETIC FIELDS
MATHEMATICS
PLANETARY IONOSPHERES
661320* - Auroral
Ionospheric
& Magnetospheric Phenomena- (1992-)