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:	https://explore.openaire.eu/search/publication?articleId=doi_________::b84b8a7464a08fea25db5db4e75a63c3 https://doi.org/10.1017/s000273160015543x Zobrazit plný text záznamu