DocumentCode
2271332
Title
Highly stable laser towards spaceborne gravitational wave detection
Author
Trobs, M. ; Hunnekuhl, M. ; Burdack, P. ; Hinze, U. ; Fallnich, C. ; Bode, M. ; Freitag, I. ; Skorupka, S. ; Heinzel, G. ; Danzmann, K.
Author_Institution
Laser Zentrum Hannover eV, Germany
fYear
2002
fDate
24-24 May 2002
Firstpage
426
Abstract
Summary from only given. The Laser Interferometer Space Antenna (LISA) is a planned spaceborne gravitational wave detector that will measure gravitational waves at millihertz frequencies. Being basically a giant Michelson interferometer with not necessarily equally spaced arm length, LISA requires an extremely stable laser source.
Keywords
Michelson interferometers; aerospace instrumentation; gravitational wave detectors; laser frequency stability; measurement by laser beam; LISA; Laser Interferometer Space Antenna; extremely stable laser source; giant Michelson interferometer; highly stable laser; planned spaceborne gravitational wave detector; spaceborne gravitational wave detection; unequally spaced arm length; Extraterrestrial measurements; Fiber lasers; Fluctuations; Frequency measurement; Laser noise; Laser stability; Optical interferometry; Orbits; Ring lasers; Temperature;
fLanguage
English
Publisher
ieee
Conference_Titel
Lasers and Electro-Optics, 2002. CLEO '02. Technical Digest. Summaries of Papers Presented at the
Conference_Location
Long Beach, CA, USA
Print_ISBN
1-55752-706-7
Type
conf
DOI
10.1109/CLEO.2002.1034160
Filename
1034160
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