Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-17T16:40:35.110Z Has data issue: false hasContentIssue false

A Southern Hemisphere Radio Meteor Orbit Survey

Published online by Cambridge University Press:  25 April 2016

G. Gartrell*
Affiliation:
Department of Physics, University of Adelaide
*
* Weapons Research Establishment, Salisbury.

Extract

A combined multi-station radar equipment of c.w. and pulse at 27 MHz was used at Adelaide (lat. 35°S) during the period December 1968 to June 1969 and again in October 1969 to measure radiants and velocities of individual meteors down to limiting radio magnitude MR = + 8. Reflections from 3 to 5 points typically separated by 2 to 6 km along each trail were used and corrections for the effects of meteor region winds and wind shears were included. To date 1667 orbits have been determined from 6 months of data.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1972

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Nilsson, C. S., Aust. J. Phys., 17, 205 (1964).Google Scholar
2 Elford, W. G., Hawkins, G. S. and Southworth, R. B., Harvard Radio Meteor Project Res. Rep. No. 11 (1964).Google Scholar
3 Verniani, F. and Hawkins, G. S., Harvard Radio Meteor Project Res. Rep. No. 5 (1964).Google Scholar
4 Verniani, F., Nuovo Cim., 33, 1173 (1964).Google Scholar
5 Verniani, F., J. Geophys. Res., 71, 2749 (1966).Google Scholar
6 Allen, H. J. and Baldwin, B. S. Jr., J. Geophys. Res., 72, 3483 (1967).Google Scholar
7 Terenteva, A. K., Smithson. Contr. Astrophys., 7, 293 (1963).Google Scholar
8 Southworth, R. B. and Hawkins, G. S., Smithson. Contr. Astrophys., 7, 261 (1963).Google Scholar
9 Hawkins, G. S., Astr. J., 67, 241 (1962).Google Scholar
10 Hasegawa, I., Index-List, General, ‘Theoretical Radiant-Points of Meteors Associated with Comets’. Institut d’Astrophysique; Documentation des Observateurs. Bull. 11, No. 1 (Fase. 3) (1958, Revis. 1962).Google Scholar