Differences between revisions 26 and 27

Lentickle model for C1

Scripts are found in iscmodeling/LentickleC1

Purpose

To get the OLTs
To get noise budget
Sensing matrix with loops

Main script to execute

C1lentickle.m builds the Optickle model, then inclides the loops defined by C1cucumber.m The Optickle model for C1 is same as Kiwamu's scripts, optC1:

optC1.m ... Optickle model
paramC1DRMI.m ... physical parameters for optC1
probesC1_00.m ... probes of the model

C1cucumber setting

Sensors
- REFL 3I1
  REFL 3Q1
  AS I2
  AS Q2
  AS DC
  AS 3I2
  AS 3Q2
Input Matrix

DoF	REFL3I1	REFL3Q1	ASI2	ASQ2	ASDC	AS3I2	AS3Q2
MICH	0	0	0	1	0	0	0
PRCL	1	0	0	0	0	0	0
SRCL	0	0	0	0	0	0	1

Output Matrix

Drive	MICH	PRCL	SRCL
IX	1	0	0
IY	-1	0	0
BS	0	0	0
PR	0	1	0
SR	0	0	1
AM	0	0	0
PM	0	0	0
OSC AM	0	0	0
OSC PM	0	0	0

Control Filters

MICH	PRCL	SRCL
ZPK(10, 1000, 1)* ZPK(5, 1, 5)	ZPK(10, 1000, 1)* ZPK(50, 1, 50)	ZPK(10, 1000, 1)* ZPK(50, 1, 50)

bodeplot of the filters These filters already have pendulum compensation. Therefore in cucumber, you don't need the pendulum compensation (mirrFilt) matrix. Here we use a flat (unity) mirrFilt.

* Mechanical transfer function dampRes = [-0.1 + 1i, -0.1 - 1i];
opt = setMechTF(opt, 'IX', zpk([], par.w * dampRes, 1 / par.mass));

Results

Frequency noise TF

Amplitude noise TF

Seismic Noise estimation (MICH)
$/!\$ preliminary

-  ⇤ ← Revision 26 as of 2012-02-16 17:32:42 → 
  Size: 2176
  Editor: KeikokokeyamaATligoDOTorg
  Comment:
+   ← Revision 27 as of 2012-02-16 18:17:29 → ⇥
  Size: 2206
  Editor: KeikokokeyamaATligoDOTorg
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
 Line 70:
+{{attachment:Feb15TF.png}}