Hostname: page-component-848d4c4894-4rdrl Total loading time: 0 Render date: 2024-07-01T11:40:05.207Z Has data issue: false hasContentIssue false
  • English
  • Français

Radar Studies of the Orbits of Small Meteoroids

Published online by Cambridge University Press:  25 April 2016

W. J. Baggaley ,
R. G. T. Bennett ,
D. I. Steel  and
A. D. Taylor
W. J. Baggaley
Affiliation:
Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand
R. G. T. Bennett
Affiliation:
Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand
D. I. Steel
Affiliation:
Anglo-Australian Observatory, Private Bag, Coonabarabran, NSW 2357 andUniversity of Adelaide
A. D. Taylor
Affiliation:
Unit tor Space Sciences, University of Kent at Canterbury, Canterbury CT2 7NR, England
Get access Rights & Permissions [Opens in a new window]

Abstract

A description is given of a radar facility operating in New Zealand which measures the atmospheric trajectories and hence heliocentric orbits of earth-impacting meteoroids having radiants with declinations +5° < δ < −30° down to a limiting radar meteor magnitude of +13 (corresponding to particle sizes of ~100 μm, masses ~10−6 g). The data handling capacity of the facility permits recording, orbit reduction and efficient presentation of orbital data using graphical packages to be carried out on a routine basis. The daily yield is ~1500 individual orbits with >3×105 secured to date; this is greater than the number determined in all previous meteoroid orbit surveys combined and forms a major southern hemisphere database for dynamical studies of the solar system meteoroid population.

Type
Solar and Solar System
Information
Publications of the Astronomical Society of Australia , Volume 11 , Issue 2 , August 1994 , pp. 151 - 156
Copyright
Copyright © Astronomical Society of Australia 1994

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

Babadzhanov, P. B. and Obrubov, Yu. V., 1992, Cel. Mech. Dynam. Astron., 54, 111.CrossRefGoogle Scholar
Baggaley, W. J., Taylor, A. D. and Steel, D. L, 1992a, In Periodic Comets, Fernandez, J. A. and Rickman, H. (eds), Universidad de la República, Montevideo, Uruguay, p.115.Google Scholar
Baggaley, W. J., Steel, D. I. and Taylor, A. D., 1992b, In Asteroids, Comets, Meteors 1991, Harris, A. and Bowell, E. (eds), Lunar and Planetary Institute, Houston, Texas, p. 37.Google Scholar
Baggaley, W. J., Steel, D. I., and Taylor, A. D., 1993, In Meteoroids and Their Parent Bodies, Štohl, J. and Williams, I. P. (eds), Astronomical Inst., Slovak Acad. Sci., Bratislava, p. 53.Google Scholar
Baggaley, W. J., Bennett, R. G. T., Steel, D. I. and Taylor, A. D., 1994, Q. J. Roy. Astron. Soc., in press.Google Scholar
Cook, A. F., Flannery, M. R., Levy, I. H., McCrosky, R. E., Sekanina, Z., Shao, C-Y., Southworth, R. B. and Williams, J. T., 1972, Meteor Research Program, NASA CR-2109, Washington D. C.Google Scholar
Drummond, J. D., 1981, Icarus, 45, 545.Google Scholar
Gartrell, G. and Elford, W. G., 1975, Aust. J. Phys., 28, 591.Google Scholar
Giese, R. H., Kneissel, B. and Rittich, U., 1986, Icarus, 68, 395.Google Scholar
Grün, E., Zook, H. A, Fechtig, H. and Giese, R. H., 1985, Icarus, 62, 244.CrossRefGoogle Scholar
Grün, E. et al, 1993, Nature, 362, 428.Google Scholar
Gustafson, B. Å. S., Grün, E., Dermott, S. F. and Durda, D. D., 1992, In Asteroids, Comets, Meteors 1991, Harris, A. and Bowell, E. (eds), Lunar and Planetary Institute, Houston, p. 223.Google Scholar
Hughes, D. W., 1987, Astron. Astrophys., 187, 879.Google Scholar
Kresák, Ľ., 1965, Smithson. Contrib. Astrophys., 11, 9.Google Scholar
Leinert, C. and Grün, E., 1990, In Physics of the Inner Heliosphere, in the series Physics and Chemistry in Space, Schwenn, R. and March, E. (eds), Springer, Heidelberg, p. 207.Google Scholar
McKinley, D. W. R., 1961, Meteor Science and Engineering, McGraw Hill, New York.Google Scholar
Nilsson, C. S., 1964, Aust. J. Phys., 17, 205.Google Scholar
Olsson-Steel, D., 1988, Icarus, 75, 64.Google Scholar
Porubčan, V., Štohl, J. and Vaňa, R., 1992, In Asteroids, Comets, Meteors 1991, Harris, A. and Bowell, E. (eds), Lunar and Planetary Institute, Houston, p. 473.Google Scholar
Steel, D. I., 1991, In IAU Colloq. 126: The Origin and Evolution of Interplanetary Dust, Levasseur-Regourd, A. C. and Hasagawa, H. (eds), Kluwer, Dordrecht, p. 299.Google Scholar
Steel, D. I., 1994, In IAU Symp. 160: Asteroids, Comets, Meteors 1993, Milani, A. Di Martino, M. and Cellini, A. (eds), Kluwer, Dordrecht, in press.Google Scholar
Weiss, A. A., 1957, Aust. J. Phys., 10, 77.Google Scholar