LIGO Document T1000247-v3
- There are three ports with in-vacuum, RF wavefront sensing. Each port requires a Gouy phase telescope to set the detector sensing matrix and to provide for good alignment. This note describes Gouy telescope solutions for the REFL, POP and AS ports.
-
- Other Files:
- Source files (GouyPhaseTelescopes.zip, file is not accessible)
DCC Version 3.4.3, contact
Document Database Administrators