Physics
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..277j&link_type=abstract
In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 277-280 (SEE N93-19113 06-90)
Physics
Diffusion, Diffusion Coefficient, Geomagnetism, Magnetic Effects, Meteor Trails, Meteoroids, Radar Echoes, Azimuth, Estimating, Height, Radar Antennas
Scientific paper
A solution to the problem of the diffusion of a meteor train in the geomagnetic field from an initial line density may be written in closed form in terms of effective diffusion coefficients depending on direction, enabling detailed calculations across the entire range of angle of train to field and relevant heights. While the effective diffusion coefficient in the plane of train and field then remains close to the zero field ambipolar value right up to 90 deg, the effective coefficient in the direction of the normal to plane of train and field drops steadily to its theta = 0 value at theta = 90 deg. At 95 km this corresponds to a change of almost 5 km, in 'diffusion height', that is, the height of an underdense meteor calculated on the basis of the exponential decay of its radar echo. We have estimated the consequent changes in the expected distribution of diffusion heights for various orientations of radar antenna and find the dependence on azimuth is very marked. The effect of the field is relatively minor for a south pointing beam but very strong if the beam is pointing north.
Jones Jason J.
Jones William
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