Ozone concentration at meteor heights determined from forward-scatter radar echoes

Details Ozone concentration at meteor heights determined from forward-scatter radar echoes Ozone concentration at meteor heights determined from forward-scatter radar echoes

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jastp..61..539c&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 61, Issue 7, p. 539-543.

Physics

1

Scientific paper

The ozone concentration has been measured in the meteor zone using a method of radar echo duration distribution suggested by Jones and Šimek (1995). Data obtained by the forward-scatter system during the Lyrid meteor shower period in five consecutive years 1992-1996 agree with the Solar Mesosphere Explorer results for the same heights of 95 km. The mean value of the ozone concentration [O3]=(1.56+/-0.05)×1014 m-3 has been derived from a total of 6596 radar meteor echoes with duration >=1 s. The results for individual years indicating a possible decrease in [O3] are discussed.

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