| Autor: |
Roger W. Romani, J. M. Rankin, D. C. Backer |
| Rok vydání: |
1992 |
| Zdroj: |
International Astronomical Union Colloquium. 128:326-328 |
| ISSN: |
0252-9211 |
| DOI: |
10.1017/s000273160015543x |
| Popis: |
We have examined high quality Arecibo data of three pulsars for evidence of strange attractors in pulse-to-pulse intensity fluctuations. Significant structure was found for PSR 0823+26, and seems related to pulse drifting and nulling activity. The low dimensionality of the possible attractor suggest that a simple dynamical model can explain this component of the flux variability. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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