Abstract
The theory relating the radio-echo rate to the incident meteor flux is extended to the case of sporadic meteors. It is shown that the relation between total influx and the echo rate observed at the equator with a suitably oriented aerial should be substantially independent of the distribution of sporadic radiants over the celestial sphere. The meteoric influx as a function of limiting magnitude (to +11 m ) has been determined from experimental data. Results for sporadic meteors and for several showers are presented.

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