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Physical and dynamical studies of meteors. Meteor-fragmentation and stream-distribution studiesPopulation parameters of 275 streams including 20 additional streams in the synoptic-year sample were found by a computer technique. Some 16 percent of the sample is in these streams. Four meteor streams that have close orbital resemblance to Adonis cannot be positively identified as meteors ejected by Adonis within the last 12000 years. Ceplecha's discrete levels of meteor height are not evident in radar meteors. The spread of meteoroid fragments along their common trajectory was computed for most of the observed radar meteors. There is an unexpected relationship between spread and velocity that perhaps conceals relationships between fragmentation and orbits; a theoretical treatment will be necessary to resolve these relationships. Revised unbiased statistics of synoptic-year orbits are presented, together with parallel statistics for the 1961 to 1965 radar meteor orbits.
Document ID
19760004830
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Sekanina, Z.
(Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Southworth, R. B.
(Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Date Acquired
September 3, 2013
Publication Date
November 1, 1975
Publication Information
Publisher: NASA
Subject Category
Space Sciences (General)
Report/Patent Number
NASA-CR-2615
Report Number: NASA-CR-2615
Accession Number
76N11918
Funding Number(s)
CONTRACT_GRANT: NAS1-11204
PROJECT: RTOP 188-45-52-03
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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