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Modeling the Input Optics with e2e
T. Findley, S. Yoshida, D. Dubois, N. Jamal, and R. Dodda
Southeastern Louisiana University
LIGO-G050219-00-D
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Objectives
Report status of e2e modeling Results
Calibrated floor motion Better Mode Cleaner Mode Matching Telescope in Detector.box
Comments/Suggestions
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Contents Estimate the table top motion for a given ground
motion. Make a Small Optic Suspension (SOS) box with
local damping, and find optimal gain settings to damp the optic when estimated table top motion is given.
Create a Mode Cleaner (MC) box, and implement the length control for the mode cleaner cavity.
Put all the optics (MCs, SM, and MMTs) in order, and create the Input Optic (IO) box.
Use the IO box in Simligo, and run the simulation for the entire detector.
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Input Optics
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Table Motion
HAM table
Vibration
isolation
stacks
Accelerometer
Suspension Point
Tower
Wire
OSEM Sensors
dtdtACCXtx )(
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HAM box
Calibrating the Table Motion
MC1 box
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ITMX pend/yaw with balanced OSEMs
Pendular Yaw
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OSEM sensor imbalance
UL
LL
UR
LR
UR= (P + Y + T) g1
UL= (P - Y + T) g2
LL= (P - Y - T) g3
LR= (P + Y - T) g4
OSEM P = UR+UL+LL+LR = (P+Y+T)g1 + (P-Y+T) g2 + (P-Y-T) g3 + (P +Y-T) g4
=(g1+g2+g3+g4)P + (g1-g2-g3+g4)Y + (g1+g2-g3-g4)T
OSEM Y = UR–UL–LL+LR = 0.1P+3.9Y+0.1T
= 0, if g1=g2=g3=g4 If g1=1.05, g2=g3=g4=0.95
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ITMX pend/yaw with pend/yaw ratio = 0.023
Pendular Yaw
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Mode Cleaner
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Mode Cleaner Continued
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MC Transmission and MC2 motion
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MC Transmitted Power
DAQE2E
Frequency Domain
Time Domain
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MC Beam Motion
Beam center 20 meters away from MC pitch (lower)
Time Domain
Frequency Domain
yaw
pitc
h
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Detector box
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Status of IO box: Contains MMT optics only
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MMT1 motion effect on CARM and DARM error signals
Time (sec)
Time (sec)
Dis
pla
cem
ent
(m o
r ra
d)
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MMT3 motion effect on CARM and DARM
Time (sec)
Dis
pla
cem
ent
(m o
r ra
d)
Time (sec)
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Power Behind ETMx due to MMT1 and MMT3 motion
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Power Behind ETMx due to MMT optics motion
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Summary
Produced a better representation of the table translational and yaw motion
Created a Mode Cleaner box with Length Sensing Control
Put the Mode Matching Telescope into Detector box
Will continue investigating the effect of table motion on the optic and the resultant beam motion
Will include Mode Cleaner box in Detector box
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Acknowledgements
People: B. Bhawal M. Evans H. Yamamoto
Organizations LIGO Livingston Observatory National Science Foundation Southeastern Louisiana University