'Noise budget' presentation slideshows

Inverted Pendulum Control for KAGRA Seismic Attenuation System

Inverted Pendulum Control for KAGRA Seismic Attenuation System. D2, Institute for Cosmic Ray Research Takanori Sekiguchi. Contents. Introduction of IP controls IP control model and simulation Current status of IP control experiment Summary. *IP = Inverted Pendulum.

719 views • 23 slides

GWA-WG1

199 views • 19 slides

Noise Budget Development for the LIGO 40 Meter Prototype

Noise Budget Development for the LIGO 40 Meter Prototype. Ryan Kinney University of Missouri-Rolla, Department of Physics, 1870 Miner Circle, Rolla, MO 65409, USA. Introduction. LIGO 40 meter prototype Transfer Functions What is a Noise Budget? Seismic Noise Example. 40m Prototype.

291 views • 18 slides

272 views • 16 slides

Phased-Array Feed Measurements at Green Bank

Phased-Array Feed Measurements at Green Bank. Karl Warnick , Brian Jeffs Jonathan Landon, Mike Elmer Roger Norrod , Rick Fisher. R&D Challenges. Technical Mutual coupling Receiver/element noise Calibration Total bandwidth Cost Drivers Receiver system complexity Signal processing.

252 views • 14 slides

MSC

118 views • 11 slides

MAIN CONTRIBUTOR NOISES

MAIN CONTRIBUTOR NOISES. SPECIFICATION PHILOSOPHY FOR NOISE ASPECTS. For the random noises, the equipments are specified : to have the photon noise as the predominant noise for the Seismology program, and as a result, all other random noises must be negligible for this program

156 views • 8 slides