Share Email Print
cover

Proceedings Paper

The Cassini gravitational wave experiment
Author(s): Salvatore F. Abbate; John W. Armstrong; Sami W. Asmar; Elias Barbinis; Bruno Bertotti; Don U. Fleischman; Mark S. Gatti; Gene L. Goltz; R. G. Herrera; L. Iess; Kyong J. Lee; Trina L. Ray; Massimo Tinto; P. Tortora; Hugo D. Wahlquist
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

Doppler tracking experiments using the earth and a distant spacecraft as separated test masses have been used for gravitational wave (GW) searches in the low-frequency band(~0.0001-0.1 Hz). The precision microwave tracking link continuously measures the relative dimensionless velocity, Δv/c, between the earth and the spacecraft. A GW incident of the systems produces a characteristic signature in the data, different from the signatures of the principal noises. For 40 days centered about its solar opposition in December 2001, the Cassini spacecraft was tracked in a search for low-frequncy GWs. Here we describe the GW experiment, including transfer functions of the signals and noises to the Doppler observable, and present noise statistics and compare them with the pre-experiment noise budget.

Paper Details

Date Published: 26 February 2003
PDF: 8 pages
Proc. SPIE 4856, Gravitational-Wave Detection, (26 February 2003); doi: 10.1117/12.458566
Show Author Affiliations
Salvatore F. Abbate, Jet Propulsion Lab. (United States)
John W. Armstrong, Jet Propulsion Lab. (United States)
Sami W. Asmar, Jet Propulsion Lab. (United States)
Elias Barbinis, Jet Propulsion Lab. (United States)
Bruno Bertotti, Univ. degli Studi di Pavia (Italy)
Don U. Fleischman, Jet Propulsion Lab. (United States)
Mark S. Gatti, Jet Propulsion Lab. (United States)
Gene L. Goltz, Jet Propulsion Lab. (United States)
R. G. Herrera, Jet Propulsion Lab. (United States)
L. Iess, Univ. degli Studi di Roma La Sapienza (Italy)
Kyong J. Lee, Jet Propulsion Lab. (United States)
Trina L. Ray, Jet Propulsion Lab. (United States)
Massimo Tinto, Jet Propulsion Lab. (United States)
P. Tortora, Univ. degli Studi di Roma La Sapienza (Italy)
Hugo D. Wahlquist, Jet Propulsion Lab. (United States)


Published in SPIE Proceedings Vol. 4856:
Gravitational-Wave Detection
Peter Saulson; Adrian M. Cruise, Editor(s)

© SPIE. Terms of Use
Back to Top