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The reasons for scatter in plots of log(inverse decay times) vs. heightfor radio meteor echoes are examined, and an explanation for thecharacteristics is offered.Effects like temperature variability, pressure variation,angular detection accuracy, pulse length, phase errors, plasma processesand variation in meteoroid metallic content are considered. Using computersimulations the observed scatter is reproduced to good accuracy,and then these results are utilized to develop a newprocedure that can be used to determine temperatures in the meteorregion. These same studies also permit determination of somelimited information about the nature of the diffusive expansionprocess and the variabilityin the metallic content of meteors.The impact of the quality of phase calibration of interferometricradars on accurate reproduction of atmospheric temperaturesis also examined

Radar meteor decay rate variability and atmospheric consequences