No CrossRef data available.
Article contents
The Annual Variation of Radio Meteor Echoes Observed from 1981 to 1985
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
The radio observations of meteor echoes using FM broadcasting were carried out from January, 1981 to June, 1985. The annual variation of meteor rates in the 5 years was obtained from the observations made from 25h through 29h in local time (16h-20h UT).
Some features in this annual variation can be explained by the occurrence of the major meteor showers. After the effects of these major showers are removed there remains a significant annual variation which shows higher rates in the winter half of the year (October to March). This seems to be caused by the annual variation of non-shower meteors radiating from the apex region.
- Type
- Meteoroids and Meteor Streams
- Information
- International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 319 - 322
- Copyright
- Copyright © Kluwer 1991
References
Suzuki, K.
et al. (1976) ‘Recording meteor echoes by FM radio’, Sky and Telescope
5, 359–362.Google Scholar
McKinley, D.W.R. (1961) Meteor Science and Engineering (McGraw-Hill Book Company, Inc., New York), 112–120.Google Scholar
Stonl, J. (1968) ‘Seasonal variation in the radiant distribution of meteors’, in Physics and Dynamics of Meteors, 298–303.Google Scholar
Hasegawa, I. (1989) in the Proceedings of Comets and Interstellar matter, 11–13 (in Japanese)Google Scholar
You have
Access