The Orbital Distribution and Origin of Meteoroids-Reference-Cited by-同舟云学术

The Orbital Distribution and Origin of Meteoroids

Published:1991 Issue: Volume: Page:291-298
ISSN:0067-0057
Container-title:Origin and Evolution of Interplanetary Dust
language:
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Author:

Steel Duncan

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-011-3640-2_62

Reference10 articles.

1. Grun, E., Zook, H.A., Fechtig, H. and Giese, R.H. (1985). ‘Collisional balance of the meteoroitic complex’, Icarus, 62, 244–272.

2. Jones, J. and Sarma, T. (1985). ‘Double-station observations of 454 TV meteors. II. Orbits’, Bull. Astron. Inst. Czechoslov., 36, 103–115.

3. Hawkes, R.L. and Jones, J. (1988). ‘Electro-optical meteor observation techniques and results’, Q. Jl. Roy. Astron. Soc, 27, 569–589.

4. Kneissel, B. and Giese, R.H. (1987). ‘The dynamics of the zodiacal dust cloud on account of optical and infrared observations’, Publ. Astron. Inst. Czechoslov. Acad. Sci., No. 67, vol. 2, 241–243.

5. Lebedinets, V.N., Korpusov, V.N. and Manokhina, A.V. (1981, 1982), ‘Radio Meteor Investigations in Obninsk: Catalogue of Orbits’, Materials of the World Data Center B, Moscow, U.S.S.R.

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