Differences between revisions 20 and 46 (spanning 26 versions)

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.

-  ⇤ ← Revision 20 as of 2011-10-07 18:03:26 → 
  Size: 2838
  Editor: TomotadaAkutsu
  Comment:
+   ← Revision 46 as of 2018-02-03 13:07:02 → ⇥
  Size: 5979
  Editor: KousekiMiyo
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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-= Optical Lever (Room Temperature) =
+= Optical Levers =
 Line 4:
-'''[[../|..Up]]'''
+'''[[KAGRA/Subgroups/AOS| back to AOS top]]'''
== 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）||[[http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/LCGT/subgroup/AOS/Meetings#m9th|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||
----
-Line 8:
+Line 18:
-Sensing local motions including --(longitudinal dof and)--
all alignment dofs (pitch, yaw and roll) of any mirrors supported by vibration isolation system.

<!> Note on the operating temperature: here the system is assumed to be utilized at room temperature, not in cryogenic temperature.
+ . 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.
-Line 15:
+Line 21:
-TBD; just see the links below.
+ . TBD; just see the links below.
-Line 20:
+Line 27:
-TBD
+ . TBD
-Line 38:
+Line 45:
-Each optical lever 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.
+ . 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 ([[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=4478|JGW-T1504478-v1]])
 . For the light source, proposed candidates are
  * superluminous LED (SLED) or
  * laser light source as LIGO.
-Line 41:
+Line 61:
-=== Light source ===
For the light source, suggested candidates are
 * superluminous LED (SLED) or
 * laser light source as LIGO.
-Line 47:
+Line 62:
-Optical fibers
+ . The optical fibers transmit the light from the source to the focusing telescope.
-Line 50:
+Line 65:
+ . TBD. Moving linear stage with micrometer and some optical components like collimators?

=== Viewport windows ===
 . See also the [[../Viewport1|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 [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1231|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/Hz^2^
 * [[KAGRA/Subgroups/AOS/DCQPDList|List of DC QPDs]]

=== Pylons ===
 . The pylons must be designed.
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+Line 82:
-TBD
+ . TBD
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+Line 85:
-TBD
+ . TBD
-Line 60:
+Line 90:
-<!> Some of the LIGO documents listed below are '''NOT''' public; to access them, you may need your own LSC account.
+ . <!> Some of the LIGO documents listed below are '''NOT''' public; to access them, you may need your own LSC account.
-Line 64:
+Line 94:
- *