Computer Science – Sound
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...284..276s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 284, no. 1, p. 276-280
Computer Science
Sound
4
Echo Sounding, Fine Structure, Flux Density, Giacobini-Zinner Comet, Meteoroid Showers, Radar Astronomy, Geminid Meteoroids, Numerical Analysis, Perseid Meteoroids
Scientific paper
Fine structure profiles of the 1985 Giacobinid meteor shower derived from the Ottawa megawatt meteor radar are presented. The recorded meteor echoes were divided for the analysis into two groups: underdense, represented by meteor echoes having durations T less than 0.4 s; and overdense, with T greater than or equal 0.4 s. Maximum activity for underdense echoes occurred at 09h 25m UT, October 8, when the ten-minute zenithal rate reached about 1200, and for overdense echoes the rate peaked at 10h 25m UT with about 700 echoes. Mass distribution factor for underdense echoes s = 2.06 and that one for overdense s = 2.11 was found.
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