Abstract:Analysis of data from recent experiments leads to the observation that the distribution of underdense meteor trail durations differs from classical predictions. A new theory for the distribution of underdense meteor trail durations has been developed based upon the assumption of a normal height distribution and lognormal amplitude distribution which leads to a lognormal distribution of the trail durations. It is shown that this model provides a better fit to observed data than the classic model. This model, ap… Show more
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