Bulletin of the American Physical Society
APS April Meeting 2019
Volume 64, Number 3
Saturday–Tuesday, April 13–16, 2019; Denver, Colorado
Session R11: Improving LIGO and Other High-Frequency Gravitational-Wave Detectors
1:30 PM–2:42 PM,
Monday, April 15, 2019
Sheraton
Room: Governor's Square 17
Sponsoring
Unit:
DGRAV
Chair: Evan Hall, Massachusetts Institute of Technology
Abstract: R11.00003 : How to Study LIGO Noise
1:54 PM–2:06 PM
Presenter:
Beverly K. Berger
(Stanford University)
Author:
Beverly K. Berger
(Stanford University)
Collaboration:
for the LIGO Scientific Collaboration
In order to increase the sensitivity of Advanced LIGO to astrophysical events, various sources of instrumental and environmental noise must be identified and ameliorated. Here we explore a single example from the LIGO Hanford instrument. On April 10, 2017, a cluster of strong glitches (transient noise events) were clearly visible in the gravitational wave channel between 16:30 and 18:30 UTC. LIGO Scientific Collaboration scientists have developed software tools to search for correlations between anomalous behavior in the gravitational wave channel and the performance recorded by the myriad of instrumental or environmental sensors operating at that time. We will show how these tools are used to identify possible causes for the observed glitches.
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2024 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700