Observations of the Vela Pulsar Using VSOP

Details Observations of the Vela Pulsar Using VSOP Observations of the Vela Pulsar Using VSOP

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aprs.conf..117g&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Scattering in the interstellar plasma acts as an AU-scale lens to resolve the emission region of the Vela pulsar. In the observer plane, scattering produces a speckle pattern. Observations of this pattern on short baselines provide a measure of the size of the source. Observations on long baselines provide information about the spatial structure of the pulsar's emission region. Observations of this pattern for the Vela pulsar are in good agreement with theory, and should provide a picture of the Vela pulsar as a function of pulse phase.

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