G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren...

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G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector Characterization Group

Transcript of G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren...

Page 1: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

G020342-00-Z

Test Mass Butterfly Modes and Alignment

Amber Bullington, Stanford University

Warren Johnson, Louisiana State University

LIGO Livingston

Detector Characterization Group

Page 2: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Introduction

How can a vibrational mode of a test mass be used for alignment?

What is the structure of a butterfly mode?

How does the detected signal from the mode vary with changing the alignment of a resonant cavity?

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The Butterfly Mode

Two orientations of this mode exist» Plus mode» Cross mode

The center of symmetry may be useful for centering a beam on a test mass

+

+-

-

+

+- -

Magnet

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Simulation of Butterfly Modes

Simulation by Dennis Coyne

Calculated Frequency of vibration = 6640.811Hz

Good Agreement with Measured Values

No mode splitting predicted

http://www.ligo.caltech.edu/~coyne/TM_modes/

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Measuring Butterfly Mode Frequencies

Drive the test mass with uniform noise» Arbitrary Waveform Generator» 6000Hz-7000Hz» Amplitude 400 counts

Lock an arm for the ETMs» Observe butterfly signal in AS_I» Turn on whitening filters AS1I, AS1Q on LSC panel» Note filters FM5 and FM6 under SUS LSC

Lock the Power Recycled Michelson for the ITMs» Observe butterfly signal in REFL_I» Turn on whitening filters AS1I,AS1Q,RFI

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Frequencies of Vibration, ETMx

Lower Mode (plus) = 6648.01Hz Upper Mode (cross) = 6648.56Hz

Amplitude Spectrum of Modes for ETMx

Page 7: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Frequencies of Vibration, ETMy

Lower Mode (plus) = 6640.217Hz Upper Mode (cross) = 6640.665Hz

Amplitude Spectrum of Modes for ETMy

Page 8: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Frequencies of Vibration, ITMx

Lower Mode = 6695.978Hz Upper Mode = 6696.391Hz

Amplitude Spectrum of Modes for ITMx

Page 9: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Frequencies of Vibration, ITMy

Only one mode seen at 6694.2Hz Degenerate Modes? Sign of Suspension Problems or Damaged Magnet? Misidentified Mode?

» ITMx and ITMy frequencies only 2Hz apart!

Page 10: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Q Measurements

Excite mode with sinusoidal drive

Stop the excitation and observe the ring down

More Q plots on 7/8/02 LLO detector group log entries

Decay of 6648.56Hz mode of ETMx

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Summary of Frequencies

Plus Mode Plus Mode Q

Cross Mode

Cross Mode Q

ETMx 6648.01Hz 2.1x106 6648.58Hz 8.3x105

ETMy 6640.217Hz 2.3x106 6640.665Hz 8.8x105

ITMx 6695.978Hz ~105 6696.391Hz ~105

ITMy NA NA 6694.16Hz ~6x103

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Determination of Mode Structure

How can the position of the nodal lines be determined?» Sinusoidal drive of desired mode» Misalign resonant cavity by known amounts

– Misalign single arm for ETMs– Misalign power recycled michelson for ITMs

» Measure signal amplitude from spectrum at different resonant configurations

Page 13: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Cavity Misalignment

Radius of Curvature

Optic Axis

Beam Displacement

ITM ETM

Page 14: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Mode Structure, ETMx

ETMx map structure suggests lower mode at 6648.01Hz has “plus” structure

Mapped with a single arm lock Map size = 23mm x 14mm

0.01

0.02

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<--Yaw from Center-->

<--

Pit

ch

fro

m C

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->

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Evidence of Plus Structure

+

+-

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Page 15: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Mode Structure, ETMy

ETMy map structure suggests upper mode at 6640.67Hz has “cross” structure

Mapped with a single arm lock initially misaligned near upper left Map size = 12mm x 8mm

0.2

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<--Yaw from Center-->

<--

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m C

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Evidence of CrossStructure

+

+- -

Page 16: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Mode Structure, ITMy

ITMy map structure suggests mode at 6694.2Hz may be a cross mode

Mapped using the Power Recycled Michelson

0.02

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<--Yaw from Center-->

<--

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Cross StructureEvidence

Anomaly

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Alignment

Butterfly mode was minimized by making slight changes in alignment

Signal did not disappear entirely Altering the alignment of the fully locked

interferometer» Signal decreased with misalignment - wrong trend!» Signal more susceptible to changes in power

Page 18: G020342-00-Z Test Mass Butterfly Modes and Alignment Amber Bullington, Stanford University Warren Johnson, Louisiana State University LIGO Livingston Detector.

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Mode Coupling

Driving one butterfly mode can excite the other mode

Sinusoidal drive of upper mode of ETMy excites lower mode

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Conclusion

What can be done in the future?» Examine the phase of the detected signal w.r.t the

drive signal» Create a “phase map”

Automated alignment with the butterfly modes?» Modes ring up naturally when full interferometer

acquires lock

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Acknowledgements

Many thanks to the staff at LIGO for a great learning experience

Special thanks to the following people» Warren Johnson» Mark Coles

National Science Foundation