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AbstractAbstract
[en] 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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Source
Mayr, H.G.; Miller, N.J.; National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center; vp; Jun 1986; vp; Thermosphere dynamics workshop; Beltsville, MD (USA); 3 Oct 1984; Available from NTIS, PC A20/MF A01
Record Type
Report
Literature Type
Conference; Numerical Data
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