Published March 1983
| Version v1
Journal article
Statistical analysis of the fine-scale time structure of PSR 1133+16
Creators
- 1. Institute for Space Research, USSR Academy of Sciences, Moscow
Description
Statistical analysis of the fine structure in the radio emission of PSR 1133+16 shows that the micropulse durations are not randomly distributed but display at least two characteristic time scales, one shorter than 250 μsec and the other between 250 μsec and roughly-equal1 msec. In more than half the pulses analyzed, the microstructure is quasiperiodic, with short (< 625 μsec) periods being distinguished from long (625--2500 μsec) periods. The microstructure time-scale and quasiperiod distributions are compared for subpulses belonging to the two separate components of the mean pulse profile
Additional details
Publishing Information
- Journal Title
- Sov. Astron. (Engl. Transl.)
- Journal Volume
- 27
- Journal Issue
- 2
- Series
- Sov. Astron. (Engl. Transl.).
- Journal Page Range
- 169-173
- ISSN
- 0038-5301
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 15023485
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ELECTROMAGNETIC PULSES; FINE STRUCTURE; PULSARS; RADIOWAVE RADIATION; STATISTICS; TIME RESOLUTION; VARIATIONS
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; MATHEMATICS; RADIATIONS; RESOLUTION; TIMING PROPERTIES
Optional Information
- Notes
- Cover-to-cover translation of Astronomicheskij Zhurnal (USSR).