O Jennrich et al 1997 Class. Quantum Grav. 14 1525 doi:10.1088/0264-9381/14/6/022
Polarization resolution of LISA
O Jennrich
, M Peterseim, K Danzmann,
and B F Schutz
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.
- PACS
-
04.30.Db Wave generation and sources
97.80.-d Binary and multiple stars
- MSC
- Subjects
- Dates
-
Issue 6 (June 1997)
Received 13 August 1996, in final form 13 January 1997
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Polarization resolution of LISA
O Jennrich et al 1997 Class. Quantum Grav. 14 1525
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W Lewandowski et al 2006 Metrologia 43 278
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On the mathematical treatment of time reversal
Michael V Klibanov and Alexandre Timonov 2003 Inverse Problems 19 1299
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