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Polarization resolution of LISA
1997
Classical and quantum gravity
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LISA is a spaceborne laser interferometer for the detection and observation of gravitational waves, currently under study by ESA. A brief introduction of the main features of this detector, concentrating on its oneyear orbital motion around the Sun is given. The amplitude as well as the phase of a gravitational wave is modulated due to that motion, allowing us to extract information from the signal. The detection of monochromatic gravitational waves based on the well-known signal detection
doi:10.1088/0264-9381/14/6/022
fatcat:7r6ooop2pzgs3de5lmd7tk6idy