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Structural peculiarities of the quadrantid meteor shower
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Isamutdinov, Sh O. Chebotarev, R. P. |
| Copyright Year | 1987 |
| Description | Systematic radio observations to investigate the Quadrantid meteor shower structure are regularly carried out. They have now been conducted annually in the period of its maximum activity, January 1 to 6, since 1966. The latest results of these investigations are presented, on the basis of 1981 to 1984 data obtained using new equipment with a limiting sensitivity of +7.7 sup m which make it possible to draw some conclusions on the Quadrantids shower structure both for transverse and lengthwise directions. |
| File Size | 2939111 |
| Page Count | 5 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19880005170 |
| Archival Resource Key | ark:/13960/t7dr7r66c |
| Language | English |
| Publisher Date | 1987-08-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Particle Flux Density Spatial Distribution Quadrantid Meteoroids Annual Variations Radar Tracking Meteoroid Showers Solar Longitude Radiometric Resolution Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |