We demonstrate feed-forward vibration isolation on a suspended Fabry-Perot interferometer using Wiener filtering and a variant of the common least mean square adaptive filter algorithm. We compare the experimental results with theoretical estimates of the cancellation efficiency. Using data from the recent Laser InterferometerGravitational Wave Observatory (LIGO) Science Run, we also estimate the impact of this technique on full scale gravitational waveinterferometers. In the future, we expect to use this technique also to remove acoustic, magnetic, and gravitational noise perturbations from the LIGOinterferometers. This noise cancellation technique is simple enough to implement in standard laboratory environments and can be used to improve...
This paper presents an adaptable, parallelizable method for subtracting linearly coupled noise from ...
We propose an adaptive denoising scheme for poorly modeled non-Gaussianfeatures in the gravitational...
The suspension noise in interferometric gravitational wave detectors is caused by losses at the top ...
Using a network of seismometers and sets of optimal filters, we implemented a feed-forward control t...
Using a network of seismometers and sets of optimal filters, we implemented a feed-forward control t...
Fluctuations in the local Newtonian gravitational field present a limit to high precision measuremen...
It is known by the experience gained from the gravitational wave detector proto-types that the inter...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
Newtonian gravitational noise from seismic fields is predicted to be a limiting noise source at low ...
Ground-based interferometric gravitational wave observatories such as Advanced LIGO must isolate the...
In this article we propose a new method for reducing Newtonian noise (NN) in laser-interferometric g...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2011.Cataloged from PDF vers...
A seismic array has been deployed at the Sanford Underground Research Facility in the former Homesta...
Standing ocean waves driven by storms can excite surface waves in the ocean floor at twice the wave ...
© 2019 American Physical Society. Interferometric gravitational-wave detectors like LIGO need to be ...
This paper presents an adaptable, parallelizable method for subtracting linearly coupled noise from ...
We propose an adaptive denoising scheme for poorly modeled non-Gaussianfeatures in the gravitational...
The suspension noise in interferometric gravitational wave detectors is caused by losses at the top ...
Using a network of seismometers and sets of optimal filters, we implemented a feed-forward control t...
Using a network of seismometers and sets of optimal filters, we implemented a feed-forward control t...
Fluctuations in the local Newtonian gravitational field present a limit to high precision measuremen...
It is known by the experience gained from the gravitational wave detector proto-types that the inter...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
Newtonian gravitational noise from seismic fields is predicted to be a limiting noise source at low ...
Ground-based interferometric gravitational wave observatories such as Advanced LIGO must isolate the...
In this article we propose a new method for reducing Newtonian noise (NN) in laser-interferometric g...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2011.Cataloged from PDF vers...
A seismic array has been deployed at the Sanford Underground Research Facility in the former Homesta...
Standing ocean waves driven by storms can excite surface waves in the ocean floor at twice the wave ...
© 2019 American Physical Society. Interferometric gravitational-wave detectors like LIGO need to be ...
This paper presents an adaptable, parallelizable method for subtracting linearly coupled noise from ...
We propose an adaptive denoising scheme for poorly modeled non-Gaussianfeatures in the gravitational...
The suspension noise in interferometric gravitational wave detectors is caused by losses at the top ...