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Parameters of microstructure and noiselike intensity fluctuation in pulsar radio emission measured with submicrosecond time resolution provided by the S2 VLBI recording/playback system

Published online by Cambridge University Press:  12 April 2016

M.V. Popov ,
V.I. Kondrat’ev ,
V.I. Altunin ,
N. Bartel ,
W. Cannon  and
A.Yu. Novikov
M.V. Popov
Affiliation:
Astro Space Center of the Lebedev Physical Institute, Profsoyuznaya 84/32, 117810 Moscow, Russia
V.I. Kondrat’ev
Affiliation:
Astro Space Center of the Lebedev Physical Institute, Profsoyuznaya 84/32, 117810 Moscow, Russia
V.I. Altunin
Affiliation:
Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109
N. Bartel
Affiliation:
York University, Department of Physics, 4700 Keele Street, North York, OntarioCanadaM3J 1P3
W. Cannon
Affiliation:
Space Geodynamic Lab, CRESTech, 4850 Keele Street, North York, OntarioCanadaM3J 1P3
A.Yu. Novikov
Affiliation:
Space Geodynamic Lab, CRESTech, 4850 Keele Street, North York, OntarioCanadaM3J 1P3

Abstract

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Three bright pulsars (B0950+08, B1133+16, and B1929+10) were observed with the 70-m radio telescope in Tidbinbilla at a frequency of 1650 MHz using the S2 Data Acquisition System which provided continuous recording of pulsar signals in two conjugate bands of B=16 MHz each. Parameters of microstructure have been analyzed using the predetection dispersion removal technique.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 179 - 180
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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