Abstract
A method of measuring the pulse arrival time of the radio emission of pulsars is described. The method is based on the use of a wideband optoelectronic processor. A special feature of the processor is a special operating mode (time delay and integration mode) of a multi-element CCD photodetector in which the dispersion of the radio emission received by the photodetector is compensated. The components of the instrumental error of the measurements are considered. Results gained from the use of the optoelectronic processor in a radio telescope are presented.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
