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On the spatial structure of the perseids meteor stream
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Rubtsov, L. N. Tarasova, I. I. Andreev, G. V. |
| Copyright Year | 1987 |
| Description | The analysis of radar observations of the Perseid meteor stream conducted in an ionospherical laboratory in the period from 1964 to 1981 is presented. The Perseids meteor rates were determined by the fluctuation method. Analysis of their hourly distributions showed that the stream maximum position is different for different years, i.e., the stream nodal position is constantly changing. The results of the analysis are presented and discussed. |
| File Size | 3520243 |
| Page Count | 5 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19880005168 |
| Archival Resource Key | ark:/13960/t8qc4x507 |
| Language | English |
| Publisher Date | 1987-08-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Spatial Distribution Flux Density Particle Emission Particle Mass Radar Tracking Meteoroid Showers Perseid Meteoroids Solar Longitude Regression Analysis Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
