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
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










