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Algebraic approach to time-delay data analysis: orbiting case
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DOI：10.1088/0264-9381/22/10/040.png)
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The laser phase noise is one of the dominant noises for the gravitational wave detector LISA. Since it is impossible to maintain equal distances among spacecraft, the time-delay interferometric (TDI) techniques are used to eliminate the laser phase noise along with optical bench noise. In this work, we estimate the effects due to the Sagnac phase by taking the realistic model for LISA orbital motion. We extend the algebraic formalism to include the effects due to the Sagnac phase.
Keyword:
INTERFEROMETRY
LISA
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3.7
论文数:
1.3W
被引数:
3.0W
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