Differences between revisions 4 and 16 (spanning 12 versions)
Revision 4 as of 2011-04-13 17:49:25
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Comment:
Revision 16 as of 2011-04-15 11:51:12
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Comment:
Deletions are marked like this. Additions are marked like this.
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=== ETM ===
 * Suspended beam reducing telescope for transmitted beam.
  * Vibration isolation requirement TBD
 * Detection optics for transmitted beam, especially QPD (suspended ? in vacuum ?), CCD
 * Optical lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended baffles to kill scattered light (suggested by Riccardo)
 * Suspended beam dumps for killing AR reflected beams.
 * CCD camera to look at the mirror surface.
Line 7: Line 20:
 * Local sensors to monitor the position of the test mass
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
 * Local sensors to monitor the position of the mirror and above masses
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z) and side
Line 15: Line 28:
=== ETM ===
 * Suspended beam reducing telescope for transmitted beam.
  * Vibration isolation requirement TBD
 * Detection optics for transmitted beam, especially QPD (suspended ? in vacuum ?)
 * Optical lever
 * Local sensors to monitor the position of the test mass
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
  * 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.
 * Suspended baffles to kill scattered light (suggested by Riccardo)
 * Suspended beam dumps for killing AR reflected beams.
 * CCD camera to look at the mirror surface.
Line 30: Line 31:
 * Detection optics for POX/POY.
 * Optical Lever
 * Local sensors to monitor the position of the mirror
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
 * Detection optics for POX/POY (2xRFPD, RFPD, DCPD, RF QPD, DC QPD, CCD)
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z) and side
Line 41: Line 42:
 * Local sensors to monitor the position of the mirror
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== Faraday ===
 * Detection optics for REFL
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.
Line 56: Line 54:
 * Local sensors to monitor the position of the mirror
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
 * Local sensors to monitor the position of the mirror and above masses
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z) and side
Line 65: Line 63:
 * Local sensors to monitor the position of the mirror
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
 * Local sensors to monitor the position of the mirror and above masses
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z) and side
Line 73: Line 71:
 * Suspended steering mirror(s) to lead the transmitted beam out of the vacuum chamber.
 * Detection optics for AS
  * AS Pick-off
  * AS RF PD/QPD (in vacuum ?)
  * Suspended mode matching telescope for OMC
  * Suspended OMC
  * In vacuum DC PD
* Optical Lever
 * Local sensors to monitor the position of the mirror
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z) and side
Line 92: Line 83:
 * Local sensors to monitor the position of the mirror
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
 * Local sensors to monitor the position of the mirror and above masses
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z) and side
Line 101: Line 92:
 * Local sensors to monitor the position of the mirror
  * At least horizontal degrees of freedom (X,Y)
  * Preferably a vertical sensor (Z)
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

----
=== MC1 ===
 * Suspended steering mirrors to lead the MC REFL beams out of the vacuum chamber.
 * Detection optics for MC REFL (RFPD, DCPD, RF QPD, DC QPD, CCD)
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== MC2 ===
 * Detection optics for transmitted beam (MCT), especially QPD (suspended ? in vacuum ?)
 * Detection optics for MCT (DCPD, DC QPD, CCD)
 * CCD to look at the MC transmitted light.
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== MC3 ===
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== MMT1 ===
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== MMT2 ===
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== Faraday ===
 * Detection optics for REFL (RFPD, DCPD, RF QPD, DC QPD, CCD)
 * CCD cameras to look at the iniput/output of FI.


----
=== OMMT1 ===
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== OMMT2 ===
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the mirror surface.

=== OMC ===
 * Suspended steering mirrors to lead the DC PD beams in the vacuum chamber.
 * Suspended steering mirrors to lead the OMC REFL beams out of the vacuum chamber.
 * Suspended steering mirrors to pickoff RF signals (1%?) out of the vacuum chamber.
 * Detection optics for In vacuum DC PD.
 * Detection optics for OMC REFL. (RFPD, DCPD, RF QPD, DC QPD, CCD)
 * Detection optics for AS RF port (RFPD, DCPD, RF QPD, DC QPD, CCD).
 * Optical Lever
 * Local sensors to monitor the position of the mirror and above masses
  * 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.
 * Suspended beam dumps for killing auxiliary beams (in vacuum).
 * CCD to look at the OMC mirror surface.


----
== Total amount ==

For IFO optics
||Item|| ||ETMX||ETMY||ITMX||ITMY||BS||PRM||PR2||PR3|| ||Total||
|| || || || || || || || || || || || ||
||CCD|| ||1||1||1||1||1||1||1||1|| ||7||
||QPD for OL|| ||2||2||2||2||2||2||2||2|| ||14||
||OL Laser|| ||2||2||2||2||2||2||2||2|| ||14||
||Local sensor|| || || || || || || || || || || ||


For input optics:
||Item|| ||MC1||MC2||MC3||MMT1||MMT2||FI|| || || ||Total||
|| || || || || || || || || || || || ||
||CCD|| ||1||1||1||1||1||2|| || || ||7||
||QPD for OL|| ||2||2||2||2||2|| || || || ||10||
||OL Laser|| ||1||1||1||1||1|| || || || ||5||
||Local sensor|| || || || || || || || || || || ||

For output optics:
||Item|| ||OMMT1||OMMT2||OMC|| || || || || || ||Total||
|| || || || || || || || || || || || ||
||CCD|| ||1||1||2|| || || || || || ||4||
||QPD for OL|| ||2||2||2|| || || || || || ||6||
||OL Laser|| ||1||1||1|| || || || || || ||3||
||Local sensor|| || || || || || || || || || || ||


For output ports:
||Item|| ||DC||OMC REFL||AP RF||REFL||POX||POY||TRX||TRY||MC REFL||MCT|| ||Total||
|| || || || || || || || || || || || || || ||
||CCD|| || ||1||1||1||1||1||1||1||1||1|| ||9||
||RF PD|| || ||1||1||1||1||1|| || ||1|| || ||6||
||2xRF PD|| || || || || ||1|| || || || || || ||1||
||PD for DC readuot|| ||1|| || || || || || || || || || ||1||
||DC PD|| || ||1||1||1||1||1|| || ||1||1|| ||7||
||DC PD high/low|| || || || || || || ||1||1|| || || ||2||
||RF QPD|| || || ||2||2||2|| || || ||2|| || ||8||
||DC QPD|| || || || || || || ||1||1|| ||1|| ||3||

For laser table:
||Item|| ||Laser||FSS REFL||FSST||PMC REFL||PMCT||MZT1||MZT2||ISS|| ||Total||
|| || || || || || || || || || || || ||
||CCD|| || ||1||1||1||1||1||1|| || ||6||
||RF PD|| || ||1|| ||1|| ||1|| || || ||3||
||DC PD|| ||2|| ||1|| ||1|| ||1||1|| ||6||
||DC QPD|| || || || || ||1|| ||1|| || ||2||

Auxiliary Optics Lists

This is a preliminary list of auxiliary optics, sensors and other stuff.

ETM

  • Suspended beam reducing telescope for transmitted beam.
    • Vibration isolation requirement TBD
  • Detection optics for transmitted beam, especially QPD (suspended ? in vacuum ?), CCD
  • Optical lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended baffles to kill scattered light (suggested by Riccardo)
  • Suspended beam dumps for killing AR reflected beams.
  • CCD camera to look at the mirror surface.

ITM

  • Optical lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended baffles (suggested by Riccardo)
  • Suspended beam dumps for AR reflected beams.
  • CCD camera to look at the mirror surface.

BS

  • Suspended steering mirrors to lead the POX/POY beams out of the vacuum chamber.
  • Detection optics for POX/POY (2xRFPD, RFPD, DCPD, RF QPD, DC QPD, CCD)
  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

PRM

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

PR2

  • Suspended steering mirror(s) to lead the transmitted beam out of the vacuum chamber.
  • Detection optics for POP.
  • Injection/Detection optics for green laser.
  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

PR3

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

SRM

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

SR2

  • Suspended steering mirror(s) to lead the green beam into the interferometer.
  • Injection/Detection optics for green laser.
  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

SR3

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.


MC1

  • Suspended steering mirrors to lead the MC REFL beams out of the vacuum chamber.
  • Detection optics for MC REFL (RFPD, DCPD, RF QPD, DC QPD, CCD)
  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

MC2

  • Detection optics for transmitted beam (MCT), especially QPD (suspended ? in vacuum ?)
  • Detection optics for MCT (DCPD, DC QPD, CCD)
  • CCD to look at the MC transmitted light.
  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

MC3

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

MMT1

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

MMT2

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

Faraday

  • Detection optics for REFL (RFPD, DCPD, RF QPD, DC QPD, CCD)
  • CCD cameras to look at the iniput/output of FI.


OMMT1

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

OMMT2

  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the mirror surface.

OMC

  • Suspended steering mirrors to lead the DC PD beams in the vacuum chamber.
  • Suspended steering mirrors to lead the OMC REFL beams out of the vacuum chamber.
  • Suspended steering mirrors to pickoff RF signals (1%?) out of the vacuum chamber.
  • Detection optics for In vacuum DC PD.
  • Detection optics for OMC REFL. (RFPD, DCPD, RF QPD, DC QPD, CCD)
  • Detection optics for AS RF port (RFPD, DCPD, RF QPD, DC QPD, CCD).
  • Optical Lever
  • Local sensors to monitor the position of the mirror and above masses
    • 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.
  • Suspended beam dumps for killing auxiliary beams (in vacuum).
  • CCD to look at the OMC mirror surface.


Total amount

For IFO optics

Item

ETMX

ETMY

ITMX

ITMY

BS

PRM

PR2

PR3

Total

CCD

1

1

1

1

1

1

1

1

7

QPD for OL

2

2

2

2

2

2

2

2

14

OL Laser

2

2

2

2

2

2

2

2

14

Local sensor

For input optics:

Item

MC1

MC2

MC3

MMT1

MMT2

FI

Total

CCD

1

1

1

1

1

2

7

QPD for OL

2

2

2

2

2

10

OL Laser

1

1

1

1

1

5

Local sensor

For output optics:

Item

OMMT1

OMMT2

OMC

Total

CCD

1

1

2

4

QPD for OL

2

2

2

6

OL Laser

1

1

1

3

Local sensor

For output ports:

Item

DC

OMC REFL

AP RF

REFL

POX

POY

TRX

TRY

MC REFL

MCT

Total

CCD

1

1

1

1

1

1

1

1

1

9

RF PD

1

1

1

1

1

1

6

2xRF PD

1

1

PD for DC readuot

1

1

DC PD

1

1

1

1

1

1

1

7

DC PD high/low

1

1

2

RF QPD

2

2

2

2

8

DC QPD

1

1

1

3

For laser table:

Item

Laser

FSS REFL

FSST

PMC REFL

PMCT

MZT1

MZT2

ISS

Total

CCD

1

1

1

1

1

1

6

RF PD

1

1

1

3

DC PD

2

1

1

1

1

6

DC QPD

1

1

2

LCGT/subgroup/ifo/MIF/AuxOpticsLists (last edited 2011-04-15 11:51:12 by OsamuMiyakawa)