Bryna Rickett

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From 2001 January to 2002 June, we monitored PSRs B0329+54, B0823+26, B1929+10, B2020+28 and B2021+51 using the Nanshan 25-m radio telescope of Urumqi Observatory to study their diffractive interstellar scintillation (DISS). The average interval between observations was about 9 days and the observation duration ranged between 2 and 6 hours depending on the(More)
Monitoring of the flux-densities near 30 GHz are reported for four pulsars. Statistically significant variations apparently random in nature are found over 10 to 20minutes, with rms amplitudes 20% to 100% of the mean flux. These fluctuations are substantially above the predictions for interstellar scintillation at these high frequencies. The observations(More)
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