EISCAT velocity patterns for theoretical plasma convection models

Details EISCAT velocity patterns for theoretical plasma convection models EISCAT velocity patterns for theoretical plasma convection models

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986thdy.work..379r&link_type=abstract

In NASA. Goddard Space Flight Center Thermosphere Dynamics Workshop, Volume 2 p 379-382 (SEE N86-29301 20-42)

Computer Science

Atmospheric Models, Convective Flow, Eiscat Radar System (Europe), Plasma Layers, Wind Velocity, Earth Ionosphere, Magnetic Poles, Universal Time, Velocity Distribution

Scientific paper

Theoretical line-of-sight velocities, as would be observed by the EISCAT radar, are computed for idealized models of plasma convection in the polar ionosphere. The calculations give the velocity as a function of range and Universal Time. For several variants of the Volland and Heelis convection models, how the maxima, minima and reversals of velocity depend on beam azimuth is examined. The analysis is designed to be applied to data from the UK-POLAR experiment, an example of which is shown.

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