VSOP Observations of PSR B0329+54

Details VSOP Observations of PSR B0329+54 VSOP Observations of PSR B0329+54

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aprs.conf..113m&link_type=abstract

Astrophysical Phenomena Revealed by Space VLBI, Proceedings of the VSOP Symposium, held at the Institute of Space and astronauti

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The pulsar B0329+54 was observed at 1.6GHz on 22 August 1998 using the HALCA satellite, the VLBA, the 140 foot telescope in Green Bank and the DSN's 70 meter telescopes in Goldstone and Madrid. The dynamic spectrum, plotting the flux versus time and frequency, shows the ``twinkling'' of the pulsars signal due to the turbulent plasma located between the pulsar and the observer. Images are made from two subsets of data, one chosen from the dynamic spectrum as it was during a multiple imaging event and could display multiple images of the pulsar and possibly image wander, and the other chosen at a time where multiple images would not be expected.

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