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Speckles in interstellar radio-wave scatteringObservations of speckles in the scattering disk of the Vela pulsar are presented and speckle techniques for studying and circumventing scattering of radio waves by the turbulent interstellar plasma are discussed. The speckle pattern contains, in a hologrammatic fashion, complete information on the structure of the radio source as well as the distribution of the scattering material. Speckle observations of interstellar scattering of radio waves are difficult because of their characteristically short timescales and narrow bandwidths. Here, first observations are presented, taken at 13 cm wavelength with elements of the SHEVE VLBI network, of speckles in interstellar scattering.
Document ID
19920073792
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Desai, K. M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Gwinn, C. R.
(California, University Santa Barbara, United States)
Reynolds, J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
King, E. A.
(Australia Telescope National Facility Epping, United States)
Jauncey, D.
(CSIRO Epping, Australia)
Nicholson, G.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Flanagan, C.
(Hartebeesthoek Radio Astronomy Observatory Krugersdorp, South Africa)
Preston, R. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Jones, D. L.
(JPL Pasadena, CA, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Subject Category
Astronomy
Meeting Information
Meeting: IAU Colloquium on Radio Interferometry: Theory, Techniques and Applications
Location: Socorro, NM
Country: United States
Start Date: October 8, 1990
End Date: October 12, 1990
Sponsors: National Radio Astronomy, IAU, International Union of Radio Science
Accession Number
92A56416
Distribution Limits
Public
Copyright
Other

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