Orionid meteor shower activity in 1979 from long-base radar observations

Details Orionid meteor shower activity in 1979 from long-base radar observations Orionid meteor shower activity in 1979 from long-base radar observations

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35....1h&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 35, no. 1, 1984, p. 1-5.

Astronomy and Astrophysics

Astronomy

5

Orionid Meteoroids, Radar Measurement, Radio Meteors, Contamination, Geminid Meteoroids, Radar Echoes

Scientific paper

The shower-to-sporadic ratios of radar meteor echo counts are derived from simultaneous radio observations at Ondřejov (Czechoslovakia), Budrio (Italy) and Gissar (USSR) during the Orionid shower period in 1979. A sharp maximum of the shower activity was observed on Oct. 23, located at 208.7° solar longitude, confirming a gradual shift of peak activity with solar longitude by 0.75 deg/year. The shower activity over the whole period is considerably higher in the range of smaller particles. A high contamination of meteor rates by ɛ Geminid shower meteors was found.

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