A note on the determination of ozone concentrations from radio-meteor duration distributions. |
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| Authors: | J Jones M Simek |
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| Institution: | (1) Department of Physics, University of Western Ontario, N6A 3K7 London, Canada;(2) Astronomical Institute, Czech Academy of Sciences, 251 65 Ondrejov, Czech Republic |
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| Abstract: | Hajduk, et al (1992) have drawn attention to a possible source of error in our earlier analysis of visual and radar observations of shower meteors from which we calculated the ozone concentration at meteor heights. We have considered their main criticism that the features of our data which we used to calculate the ozone concentration may have been due to the constraint that our meteors had to be observed by both methods. We have shown that observations collected from radar-only systems show very similar characteristics and that these can be analysed without recourse to visual data to produce very similar results to those from our original analysis.
Presented at theInternational Conference on  Meteoroids 23 – 31 August 1994 in Bratislava.Submitted to Earth, Moon and Planets |
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| Keywords: | meteors radio-meteors meteor streams ozone |
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