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<!> Some of the LIGO documents listed below are '''NOT''' public; to access them, you may need your own LSC account.

Optical Lever (Room Temperature)

Related subgroups: VIS, IOO, MIF, VAC, CRY...


..Up

Scope

Sensing local motions including longitudinal dof and all alignment dofs (pitch, yaw and roll) of any mirrors supported by vibration isolation system.

<!> Operating temperature: here the system is assumed to be utilized at room temperature, not in cryogenic temperature.

Applicable Documents

General Description

Receiver and Transmitter

Naming Conventions

TBD

Locations

  • BS chamber
  • ITM chambers (X,Y)
  • ETM chambers (X,Y)
  • PRC chambers (dummyPRC, PR2, PR3)
  • SRC chambers (dummySRC, SR2, SR3)
  • MC chambers (MC1, MC2...)

Requirements

  • Sensor noise should be less than xxx.
  • Sensor's dynamic range should be greater than xxx.
  • At least horizontal degrees of freedom (X,Y)
  • Preferably a vertical sensor (Z) and side
  • The sensors have to be rigidly mounted on the ground so that these are useful for remembering the position of the mirror and recording the drifts.

Characteristics

TBD

Inspection plans

TBD

Procurement process and plans

TBD

<!> Some of the LIGO documents listed below are NOT public; to access them, you may need your own LSC account.

LCGT/subgroup/AOS/OptLev1 (last edited 2018-02-03 13:07:02 by KousekiMiyo)