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Comparison of atmospheric delay statistics from Deep Space Network arrays and nearby test interferometers

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dc.contributor.author Morabito, David D.
dc.contributor.author D'Addario, Larry
dc.contributor.author Finley, Susan G.
dc.date.accessioned 2019-06-11T20:25:05Z
dc.date.available 2019-06-11T20:25:05Z
dc.date.issued 2016-10-17
dc.identifier.citation 22nd Ka and Broadband Communications Conference, Cleveland, Ohio, October 17-20,2016 en_US
dc.identifier.clearanceno 16-4008
dc.identifier.uri http://hdl.handle.net/2014/46230
dc.description.abstract In this paper, we report on the results of additional array demonstrations involving the Kepler spacecraft and compare the adjusted STI phase fluctuations with those seen by a nearby two-element array of 34 m diameter antennas tracking Kepler’s 32 GHz signal at the Goldstone, California and Madrid, Spain DSN sites. We also discuss results from a demonstration using an array over a longer 12.5 km baseline. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2016 en_US
dc.title Comparison of atmospheric delay statistics from Deep Space Network arrays and nearby test interferometers en_US
dc.type Preprint en_US


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