Radar meteor orbital structure of Southern Hemisphere cometary dust streams

Details Radar meteor orbital structure of Southern Hemisphere cometary dust streams Radar meteor orbital structure of Southern Hemisphere cometary dust streams

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc...33b&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 33-36 (SEE N93-19113 06-90)

Computer Science

Graphics

2

Comets, Computer Graphics, Cosmic Dust, Fine Structure, Meteoroids, Orbital Elements, Radar Astronomy, Southern Hemisphere, Streams, Data Reduction, Radar Data, Radio Signals, Signal Processing

Scientific paper

The Christchurch, New Zealand meteor orbit radar (AMOR) with its high
precision and sensitivity, permits studies of the orbital fine structure
of cometary streams. PC generated graphics are presented of data on some
Southern Hemisphere Streams. Such data can be related to the formation
phase and subsequent dynamical processes of dust streams.

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