Very long baseline interferometry observations using the tracking and data relay satellite as an orbiting radio telescopeAn antenna in geostationary orbit was used for VLBI observations at 2.3 GHz, in combination with ground antennas in Australia and Japan. 23 of the 25 observed sources were detected on orbiter-ground baselines, with baseline lengths as large as 2.15 earth diameters. Brightness temperatures between 10 to the 12th K and 4 x 10 to the 12th K were measured for 10 sources.
Document ID
19890026402
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Linfield, R. P. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Levy, G. S. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Ulvestad, J. S. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Edwards, C. D. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Jordan, J. F., Jr. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Dinardo, S. J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Christensen, C. S. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Preston, R. A. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Skjerve, L. J. (California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Blaney, K. B. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Subject Category
Astronomy
Meeting Information
Meeting: IAU Symposium on the Impace of VLBI on Astrophysics and Geophysics