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The gravitational wave detection experiment: Description and anticipated requirementsThe experiment to detect gravitational waves in ultraprecise two-way Doppler data is described, as are the anticipated requirements for the Deep Space Network, the spacecraft, and the data processing system. The special feature which allows the usage of ultraprecise Doppler data for the possible detection of gravitational waves is a unique three-pulse signature which is a function of the spacecraft, earth, and gravitational wave propagation direction geometry. The pulses (fractional frequency shifts) result from effects which are conveniently described as follows: Clock speed-up (earth only effect) and buffeting (equal earth and spacecraft effect).
Document ID
19780024211
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Berman, A. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 9, 2013
Publication Date
August 15, 1978
Publication Information
Publication: The Deep Space Network
Subject Category
Geophysics
Accession Number
78N32154
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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