Observation of cosmic radio beacons by the method of radio interferometry with very long base lines

Details Observation of cosmic radio beacons by the method of radio interferometry with very long base lines Observation of cosmic radio beacons by the method of radio interferometry with very long base lines

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..632g&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, July-Aug. 1980, p. 632-642. In Russian.

Astronomy and Astrophysics

Astronomy

Extragalactic Radio Sources, Radio Beacons, Radio Frequency Interference, Satellite-Borne Instruments, Very Long Base Interferometry, Computerized Simulation, Frequency Analyzers, Geodynamics, Satellite Observation, Time Lag

Scientific paper

An important feature of radio interferometry with very long base lines, from the astronomical point of view, is the feasibility of determining precisely the absolute values of the coordinates of extragalectic cosmic radio sources (beacons) from satellites or the moon. Some theoretical aspects of such determinations are examined, and a computer simulation is performed to study the potentialities of VLBI for such purposes.

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