Differences between revisions 45 and 46

Optical Levers

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

Action Items

A/I化できたもの、されたもののリスト

AI_AOS_OPLEV#	Identified on	Assigned to	Status	Description
001 仕様の確認	20120401	Michimura	Closed（20120427）	議事録など参照。一応これはこれでclosedということにしておく。
002 プロトタイプ設計、製作、テスト	20120401	Agatsuma, Takahashi	進行中	光源の選定、寿命の確認。Detectorの選定、線形性の確認etc。ちゃんと列挙した方がいいのだけれども。
003 光学系の概念設計	20121112	Agatsuma, Takahashi	進行中	光てこの設置位置を確定すべく、まずはどのくらいの占有空間が真空槽の外側に必要かを把握するため。光てこ系の光学系概念図をつくる。部品選定が未定の部分は両方に対応できるようにしておく。（光学素子の型番や素子間の距離も記入のこと）。（光源）→（レンズ）→viewport、、、といったものでよい。
004 実装図へ落としこむ	20121112	Akutsu?		AI003の光学系概念図を、真空槽近くの置き場のスペースにあうように実装図に落としこむ（もしくは占有されるスペースをわりだす、くらいでもいいのかもしれません）これは、みんなであつまってちょっと議論が必要かもです。
005 CADへ反映	20121112	????		AI004の結果を、台座、足場ふくめてCADに反映

Contents

Optical Levers

Scope

The scope of optical levers is to sense local angular motions (pitch and yaw) of any mirrors supported by vibration isolation system and other suspended stuffs including suspeded optical benches.

Applicable Documents

TBD; just see the links below.

General Description

Naming Conventions

Locations

BS chamber
ITM chambers (X,Y)
ETM chambers (X,Y)
PRC chambers (PRC, PR2, PR3)
SRC chambers (SRC, 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

Each optical lever consists of an optical system, a frontend circuit, and a human interface software.
The optical system consists of the following parts: a light source, optical fibers, a focusing telescope, viewport windows, a detector, and pylons which support the focusing telescope and the detector.

The frontend circuit is TBD. Maybe we need analog cables (and what kind of connector should we use?), whitening filters and antialiasing filters. Maybe the matrix circuit will be realized using the digital systems, but in commissioning phase, we will need analog matrix.

The human interface software is TBD, which shows the mirrors' dofs monitored by Optical Levers.

Light source

SLD-MS-261-MP1-FC/APC-PMF (from SUPERLUM)
- P = 1mW, approximately
- lambda = 670 nm, typically.
- A lab test with the collimator and focuser at NAOJ (JGW-T1504478-v1)
For the light source, proposed candidates are
- superluminous LED (SLED) or
- laser light source as LIGO.

Optical Fibers

The optical fibers transmit the light from the source to the focusing telescope.

Focusing Telescopes

TBD. Moving linear stage with micrometer and some optical components like collimators?

Viewport windows

See also the viewport subsystem.
It should be transparent for the light source wavelength.
There should be no wedge; otherwise the multiple spots of light would be problematic.
See JGW-T1201231, Effect due to viewports for optical lever (in Japanese)

Detectors

The detector will be an ordinary quadruplet photocondutive circuit with QPD. The noise level at xxx Hz should be xxx m/Hz²
List of DC QPDs

Pylons

The pylons must be designed.

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-Deletions are marked like this.
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- * SLD-MS-261-MP1-FC/APC-PMF (from )
+ * SLD-MS-261-MP1-FC/APC-PMF (from SUPERLUM)
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+   * A lab test with the collimator and focuser at NAOJ ([[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=4478|JGW-T1504478-v1]])