Wide Angle Scatter from ETM HR
- Document #:
- LIGO-T1200425-v1
- Document type:
- T - Technical notes
Other Versions:
- Abstract:
- The displacement noise, m/rtHz @ 100 Hz, caused by re-scattering of wide-angle scattered light from the H1 ETMX was determined by using the ZEMAX ray trace detector and the scattering cross-section reciprocity theorem of Flanagan-Thorne; the displacement noise meets the SLC requirement.
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- Referenced by:
- LIGO-E1300319: Arm Cavity Baffle (ACB) supporting analyses/models
- LIGO-E1300345: Repository for ACB Baffle Supporting Analyses/models