JPL VLBI Group Report for 1998-1999
This report describes the transitional activities of the JPL Analysis Center.
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This report describes the transitional activities of the JPL Analysis Center.
Contents include the following: 1.Observation coordination. 2. Data acquisition system control software. 3. Station support. 4. Correlation, data processing, and analysis. 5. Data distribution and archiving. 6. Technique improvement and research. 7. Computer support.
The Mars Exploration Rover mission plans to launch two spacecraft, each containing one rover, and to deliver them to the surface of Mars allowing the rovers to collect science data on the surface.
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The physical conditions in the inner parsec of accretion disks believed to orbit the central black holes in active galactic nuclei can be probed by imaging the absorption of background radio emission by ionized gas in the disk.
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We present high-resolution very long baseline interferometry images of three southern radio sources that the Energetic Gamma-Ray Experiment Telescope (EGRET), on board the Compton Gamma Ray Observatory, has identified as greater than 100 MeV gamma-ray sources.
The strong radio source PKS 1830-211 consists of two compact components located on opposite sides of a fainter ring of radio emission 1 arcsecond in diameter.
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Measurement of the displacement of a radio-emitting star around the barycenter of a possible planetary system can be carried out by astrometric.
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In this paper the design and performance of a single screen frequency selective surface with gridded square loop patch elements are described for diplexing the X-and Ku-band signals in an Orbiting Very Long Baseline Interferometer (OVLBI) earth station reflector antenna system.
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