IfoCAD simulations for TTL noise analyses in LISA @LISAcommunity
IfoCAD simulations for TTL noise analyses in LISA  @LISAcommunity
Uploaded July 2022 | Updated September 2026, 1 hour ago
A major contributor of noise in LISA is the so-called tilt-to-length coupling (TTL). This is the path length signal noise induced by angular and lateral jitters in an interferometric setup. In our talk, we will present various TTL noise simulations conducted using IfoCAD, an in-house interferometry analysis tool. These simulations include TTL noise in the test mass interferometers and the inter-satellite interferometers, caused by the jitter of the transmitting and receiving spacecraft. Additionally, we will discuss the plan and status of simulations using LISA's latest optical design.

Authors:
Ms Megha Dave (Presenting)
AEI, Hannover, Germany
Mr Rodrigo Garcia Alvarez (Presenting)
AEI, Hannover, Germany
IfoCAD simulations for TTL noise analyses in LISALISA Symposium XIV Parallel A LISA Instrumentation 3 Part 2LISA Symposium 2026 - Parallel 5-BLPF - A Space Saga Part 6Experimental backscatter measurement rig for LISA beam dumps and FIOS characterisationAbout the modes and tones of Black Hole RingdownsLISA Symposium XIV Day 1 Plenary Block 1 CompletePredictions for Ultra Compact X-Ray Binaries from Combined GW and Electromagnetic Wave ObservationsTesting of a First-Generation Optical Truss Interferometer for the LISA TelescopeRF differential phase measurements of the LISA fiber amplifierProspecting the precision of massive black hole spectroscopy with LISAThe James Webb Space Telescope - Gillian Wright (UK ATC)
LISA Mission |

IfoCAD simulations for TTL noise analyses in LISA

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