Published August 1987
| Version v1
Report
Spatial structure of the Perseids meteor stream
Creators
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
Additional details
Publishing Information
- Imprint Title
- Middle atmosphere program. Handbook for MAP, volume 25
- Journal Page Range
- vp.
- Report number
- N--88-14502
Conference
- Title
- 1. GLOBMET symposium on middle atmosphere program.
- Dates
- 19-24 Aug 1985.
- Place
- Dushanbe (USSR).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19082550
- Subject category
- S58: GEOSCIENCES;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- EXPERIMENTAL DATA; FLUX DENSITY; METEOROIDS; REGRESSION ANALYSIS; SPATIAL DISTRIBUTION
- Descriptors DEC
- DATA; DISTRIBUTION; INFORMATION; MATHEMATICS; NUMERICAL DATA; STATISTICS