Scintillation observations of PSR B0823+26
arXiv:1310.8076 · doi:10.1093/mnras/stt1750
Abstract
We present results of the analysis of interstellar scintillation in PSR B0823+26. Observations were conducted at a frequency of 1.7 GHz using the 32-m Torun Centre for Astronomy radio telescope. More than 50 observing sessions, lasting on average 10 h, were conducted between 2003 and 2006. We found interstellar scintillation parameters by means of dynamic spectrum analysis as well as structure function analysis of the flux density variations. We identified two distinctive time-scales, which we believe to be the time-scales of diffractive and refractive scintillation. Our results show that at the given frequency the diffractive time-scale in PSR B0823+26 is min, the refractive time-scale is min and the decorrelation bandwidth is MHz.
9 pages, 2 tables, 5 figures, accepted for publication in MNRAS
References in corpus (1)
Cited by in corpus (9)
- The analysis of the largest sample of multi-frequency pulsar scatter time estimates
- Pulsar scintillation studies with LOFAR. I. The census
- Radio emission features in different modes of PSR J0826+2637 (B0823+26)
- The study of multi-frequency scattering of ten radio pulsars
- Scattering study of Pulsars below 100 MHz using LWA1
- Pulsar Scintillation Studies with LOFAR: II. Dual-frequency scattering study of PSR J0826+2637 with LOFAR and NenuFAR
- The Pulsar Science Collaboratory: Multi-Epoch Scintillation Studies of Pulsars
- Scintillation Bandwidth Measurements from 23 Pulsars from the AO327 Survey
- Study of the variability and components of the pulsar B0823+26 at a frequency of 111 MHz