Wide Angle Scatter from ETM HR

Document #:

LIGO-T1200425-v1

Document type:

T - Technical notes

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.

Files in Document:

• T1200425_Wide angle Scatter from ETM Test Mass.pdf (file is not accessible)

Other Files:

• T1200425_Wide angle Scatter from ETM Test Mass.docx (file is not accessible)

Topics:

• Auxiliary Optics
• Final Design

Authors:

• Michael Smith

Keywords:

SLC ETM-ACB Photon Cal

Referenced by:

• LIGO-E1300319: Arm Cavity Baffle (ACB) supporting analyses/models
• LIGO-E1300345: Repository for ACB Baffle Supporting Analyses/models