2019
DOI: 10.1088/1361-6382/ab3a16
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LISA telescope: phase noise due to pointing jitter

Abstract: In a space based gravitational wave antenna like LISA, involving long light paths linking distant emitter/receiver spacecrafts, signal detection amounts to measuring the light-distance variations through a phase change at the receiver. This is why spurious phase fluctuations due to various mechanical/thermal effects must be carefully studied. We consider here a possible pointing jitter in the light beam sent from the emitter. We show how the resulting phase noise depends on the quality of the wavefront due to … Show more

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Cited by 12 publications
(18 citation statements)
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“…Unfortunately, the mirrors building the telescope are not perfect and distortions of the phase surface, called aberrations, exist. It has been shown [4] that those defects, coupled with mispointing and fluctuations (jitter) can cause a phase noise at reception. It is essential to assess this noise and compare it to the sensitivity level required by LISA.…”
Section: Theorymentioning
confidence: 99%
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“…Unfortunately, the mirrors building the telescope are not perfect and distortions of the phase surface, called aberrations, exist. It has been shown [4] that those defects, coupled with mispointing and fluctuations (jitter) can cause a phase noise at reception. It is essential to assess this noise and compare it to the sensitivity level required by LISA.…”
Section: Theorymentioning
confidence: 99%
“…Δ is the disk of radius a in the plane z=0. We now consider, as we did in our preceding paper [4], that the beam is emitted with a mispointing error that contains both a static value defined by the angles (θ 0 , ψ 0 ), and a dynamic jitter defined by angles (θ 1 (t), ψ 1 (t)). This gives an additional phase factor in equation (2): with dy y y º -0 1 .…”
Section: Theorymentioning
confidence: 99%
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