A new passive seismic attenuation system is being developed to replace the current passive attenuation stacks in LIGO 2, it is expected to drive the seismic contribution to the interferometer noise below any other noise source. The SAS will be effective completely starting at about 5 Hz, well inside the (uncompensated) gravity gradient noise wall
To meet the overall isolation and alignment requirements for the optics in Advanced LIGO, the planne...
Reducing the impact of seismic activity on the motion of suspended optics is essential for the opera...
L'étude présentée porte sur le contrôle actif des supensions pour Advanced LIGO. LIGO est un projet ...
The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device expressly d...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
Isolation from seismic motion is vital for vibration sensitive experiments. The seismic attenuation ...
Multiple-stage seismic vibration isolation stacks, which consist of alternating layers of stiff mass...
Abstract. Both present LIGO and advanced LIGO (Ad-LIGO) will need an output mode cleaner (OMC) to re...
The current interferometric gravitational wave detectors are being upgraded to what are termed ''sec...
TAMA300 has been upgraded to improve the sensitivity at low frequencies after the last observation r...
The seismic isolation needed for LIGO-II will require a dramatic technological change from the passi...
AbstractThe current interferometric gravitational wave detectors are being upgraded to what are term...
Gravitational wave detectors aim to detect strain perturbations of space-time on the order of 10^-21...
The second/third generation interferometric gravitational wave detectors need not only strong attenu...
To meet the overall isolation and alignment requirements for the optics in Advanced LIGO, the planne...
Reducing the impact of seismic activity on the motion of suspended optics is essential for the opera...
L'étude présentée porte sur le contrôle actif des supensions pour Advanced LIGO. LIGO est un projet ...
The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device expressly d...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
Isolation from seismic motion is vital for vibration sensitive experiments. The seismic attenuation ...
Multiple-stage seismic vibration isolation stacks, which consist of alternating layers of stiff mass...
Abstract. Both present LIGO and advanced LIGO (Ad-LIGO) will need an output mode cleaner (OMC) to re...
The current interferometric gravitational wave detectors are being upgraded to what are termed ''sec...
TAMA300 has been upgraded to improve the sensitivity at low frequencies after the last observation r...
The seismic isolation needed for LIGO-II will require a dramatic technological change from the passi...
AbstractThe current interferometric gravitational wave detectors are being upgraded to what are term...
Gravitational wave detectors aim to detect strain perturbations of space-time on the order of 10^-21...
The second/third generation interferometric gravitational wave detectors need not only strong attenu...
To meet the overall isolation and alignment requirements for the optics in Advanced LIGO, the planne...
Reducing the impact of seismic activity on the motion of suspended optics is essential for the opera...
L'étude présentée porte sur le contrôle actif des supensions pour Advanced LIGO. LIGO est un projet ...