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ligo interferometrycontroller range: ~100 µm (tides) control of diff. arm length: ≤10-13 m rms laser intensity noise: ≤10-7 /√hz at 150 hz frequency noise:
mission/study namelsc/virgo meeting, baton rouge march 19-22, 2007 optics working group jerald a. britten, hoang t. nguyen, james d. nissen, cindy c. larson, michael d. aasen,
slide 1july 20, 2004 middletown ct ligo-g050323-00-0 accelerating masses create ripples in space-time need astronomical sized masses moving near speed of light to get detectable
lane community college j brau june 11 2002 1 gravity waves: a new way of searching for black holes and other exotic astrophysical oddities jim brau center for high energy…
electronic speckle interferometry, phase-mapping, and nondestructive testing techniques applied to real-time, thermal loading jianmin wang and ian grant a digital phase-mapping…
mission/study namelsc/virgo meeting, baton rouge march 19-22, 2007 optics working group jerald a. britten, hoang t. nguyen, james d. nissen, cindy c. larson, michael d. aasen,
advanced ligo ligo-t0900239-v1 1 ligo laboratory ligo scientific collaboration ligo-t0900239-v1 advanced ligo xxx aos: optical lever and viewport conceptual design eric black…
ligo m060056-v2 1 ligo laboratory ligo scientific collaboration ligo-m060056-v2 advanced ligo 22 march 2011 advanced ligo reference design advanced ligo team this is an internal…
ligo and advanced ligo: technical issues dave ottaway (for ligo scientific community) ligo lab kavli institute for astrophysics and space research, massachusetts institute…
no slide titleligo-g030009-00-w ligo’s mission is to open a new portal on the universe in 1609 galileo viewed the sky through a 20x telescope and gave birth to modern
laser interferometer gravitational wave observatory laser interferometer gravitational wave observatory advanced ligo ligo-t00xxxx-xx-d 12 ligo laboratory ligo scientific…
ajw, caltech, ligo project 1ligo-g000165-00-r physics of ligo lecture 2 last week: § ligo project § gw physics, astrophysical sources § principles of gw ifo’s this week:…
ligo-g020481-00-m ligo overview barry barish nsf annual review 23-oct-02 ligo laboratory 2 ligo-g020481-00-m ligo schedule and plan 1996 construction underway mostly civil…
ligo detector performance & commissioning17 november, 2003 at ligo livingston observatory ligo-g030564-05-d 5 mirror separations are integer half-wavelength multiples
powerpoint presentationfor gravitational waves ligo laboratory gravitational waves gravitational waves are disturbances in the curvature of space-time caused by the motions
first ligo search for binary inspirals peter shawhan (ligo lab / caltech) ligo pac meeting june 6, 2003 peter shawhan (ligo/caltech) executive summary we searched for inspiral…
slide 1ligo-g020012-01-w ligo commissioning status reported on behalf of ligo colleagues by fred raab, ligo hanford observatory slide 2 ligo-g020012-01-w raab: ligo commissioning…
no slide titleligo-g080597-00-w outline what nsf decided we wanted to do… what we did… ligo-g080597-00-w fred raab, chair cindy akutagawa, ligo lab contact
no slide titlefred raab, ligo detector commissioning some of the technical challenges typical strains < 10-21 at earth ~ 1 hair’s width at 4 light years understand
sentinel-1 toolbox copyright © 2020 skywatch space applications inc. https:skywatch.co http:step.esa.int stripmap interferometry tutorial issued may 2015 updated august…