Ligo observatory
[DOC File]Laser Interferometer Gravitational Wave Observatory
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2 Laser Interferometer Gravitational Wave Observatory . ERMX. ERMY *Note: design of the S/PR telescope configuration has significantly evolved. For up to date details see current documentation in LIGO-T0900043-v11. Figure 2 Influence of round trip arm cavity fundamental mode loss on the interferometer performance.
[DOC File]The tiltmeter controls contain a constant called the ...
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LIGO Laboratory / LIGO Scientific Collaboration. LIGO-T1000340-v1 LIGO March 20, 2010. Tiltmeter Characterization. Amanda O’Toole, Abhik Bhawal, Morgan Asadoor, Riccardo DeSalvo. Distribution of this document: LIGO Scientific Collaboration. This is an internal working note. of the LIGO Laboratory. California Institute of Technology. LIGO ...
[DOC File]Laser Interferometer Gravitational Wave Observatory
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E-mail: info@ligo.caltech.edu Massachusetts Institute of Technology. LIGO Project – NW17-161. 175 Albany St. Cambridge, MA 02139. Phone (617) 253-4824. Fax (617) 253-7014. E-mail: info@ligo.mit.edu LIGO Hanford Observatory. P.O. Box 1970. Mail Stop S9-02. Richland WA 99352. Phone 509-372-8106. Fax 509-372-8137 LIGO Livingston Observatory. P.O ...
[DOC File]ws-procs9x6
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The LIGO Hanford Observatory (LHO) in Washington State has two laser interferometers called H1 and H2. The LIGO Livingston Observatory (LLO) in Louisiana has a single interferometer called L18. In the fifth science run of LIGO, the total data acquisition rate of three interferometers exceeded 16Mb/s9.
[DOC File]Laser Interferometer Gravitational Wave Observatory
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“LIGO interferometer operating at design sensitivity with application to gravitational radiometry,” Stefan Ballmer, Ph.D thesis, MIT, 2006, section 2.8.4. K. Goda et al., “Frequency Resolving Spatiotemporal Wavefront Sensor,” Optics Letters 29, pp.1452-1454 (2004) LIGO LIGO-M070109-02-R. 5 Laser Interferometer Gravitational Wave Observatory
The Effect of Transverse Shifts on the LIGO interferometer
The Laser Interferometer Gravitational-Wave Observatory (LIGO) is an ongoing project to measure the gravitational radiation predicted by general relativity. According to Albert Einstein’s theory of general relativity, gravity can be thought of as a curvature of space-time.
[DOC File]Paper Title (use style: paper title)
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LIGO has two observatory sites (H and L) in the United States with a total of three laser interferometers (H1, H2 and L1). In addition to the two observatory sites in United States, LIGO also collaborates the British-German GEO [9] 600m detector located near Hannover, Germany; and shares data with the Italian/French VIRGO [10] detector.
[DOC File]Laser Interferometer Gravitational Wave Observatory
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LIGO Vacuum Compatibility, Cleaning Methods and Procedures, LIGO-E960022-00-D. ASC Optical Lever Design Requirement Document, LIGO-T950106-01-D. LIGO-E000007-00. LIGO Naming Convention (LIGO-E950111-A-E) LIGO Project System Safety Management Plan LIGO-M950046-F. LIGO EMI Control Plan and Procedures (LIGO-E960036)
[DOC File]Laser Interferometer Gravitational Wave Observatory
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LIGO-T050226-00-D, “Faraday Isolator Specifications for Advanced LIGO”, D.H. Reitze, et al. The H2 FI was replaced in 2003; the H2 FI assembly weighs more than the older H1 and L1 FIs. “Analysis of Stray Magnetic Fields from the Advanced LIGO Faraday Isolator”, T060025-00-D, G. Mueller, et al
[DOC File]SEISMOLOGY
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Figure 1: March 11, 2011 Japan magnitude 9.0 earthquake as seen on a seismometer at LIGO Hanford Observatory. Tell students the x axis is time in a 24-hour clock and the y axis is frequency in waves per second (Hertz). Ask them to compare this seismogram with the ones they have studied in the unit so far.
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