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  Polarization resolution of LISA

Jennrich, O., Peterseim, M., Danzmann, K., & Schutz, B. F. (1997). Polarization resolution of LISA. Classical and Quantum Gravity, 14(6), 1525-1529. doi:10.1088/0264-9381/14/6/022.

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Jennrich, O.1, Author
Peterseim, M.1, Author
Danzmann, K.2, Author           
Schutz, B. F.3, Author           
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1External Organizations, Institut für Atom- und Molekülphysik, Universität Hannover, Appelstraße 2, 30167 Hannover, Germany, ou_persistent22              
2Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_24010              
3Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              

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 Abstract: We discuss LISA's ability to resolve different polarizational states of a gravitational wave with fixed frequency and amplitude. Assuming a binary as the source of the gravitational wave, its orientation is connected with the polarization of the gravitational wave emitted. Using methods of signal processing, we calculate the 1- uncertainty range for measuring the orientation of the source.

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 Dates: 1997-06
 Publication Status: Published online
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 Rev. Type: Peer
 Identifiers: DOI: 10.1088/0264-9381/14/6/022
eDoc: 328688
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Title: Classical and Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 14 (6) Sequence Number: - Start / End Page: 1525 - 1529 Identifier: ISSN: 0264-9381