Observations of PSR 0950 + 08 at 103 MHz

Abstract

n this article we report the possible cause of an enormously large enhancement (burst) in the ratio flux of PSR 0950 + 08. The burst was observed by two radio telescopes at Rajkot and Thaltej separated by 20 km. Simple folded data and cross correlogram brings out clearly the period of pulsar and indicate that the radio pulses remained intact in spite of their passage through the interplanetary medium. We argue that this burst is intrinsic to the source and not caused by the intervening medium.