The character of pulse delays during radio bursts in the pulsar B0943+10
- Authors: Suleymanova S.A.1, Pugachev V.D.1
- 
							Affiliations: 
							- Pushchino Radio Astronomy Observatory, Astro Space Center
 
- Issue: Vol 61, No 5 (2017)
- Pages: 428-439
- Section: Article
- URL: https://journals.rcsi.science/1063-7729/article/view/190721
- DOI: https://doi.org/10.1134/S1063772917050080
- ID: 190721
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Abstract
Results of a new series of observations of the anomalous pulsar B0943+10 carried out on the Large Scanning Antenna and DKR-1000 radio telescope of the Pushchino Radio Astronomy Observatory at 112 and 62 MHz, respectively, are presented. Several hundred pulse-arrival times (PATs) obtained on various days in 2013–2016 that correspond to the burst (B) mode emission are analyzed. A method for establishing the many-hour pulse shift in the emission window from 3.5-minute fragments is proposed. The delay of the mean pulse relative to the pre-calculated value follows an exponential law with a relaxation time of about 47 minutes. The pulse delay grows by 6 ms during the five hours following the onset of a burst. The random scatter of the residual PAT deviations is comparable to the amplitude of the systematic variations in these times over the lifetime of the B mode. These observations show that the character of the pulse delay as a function of time is the same at 112 and 62 MHz.
About the authors
S. A. Suleymanova
Pushchino Radio Astronomy Observatory, Astro Space Center
							Author for correspondence.
							Email: suleym@prao.ru
				                					                																			                												                	Russian Federation, 							Pushchino						
V. D. Pugachev
Pushchino Radio Astronomy Observatory, Astro Space Center
														Email: suleym@prao.ru
				                					                																			                												                	Russian Federation, 							Pushchino						
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