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LIGO-G050217-00-Z 1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU I. Pre-S4 “fixes” II.Some S4 veto issues III. Early coupling results from S4 PEM injections
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LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

Jan 18, 2016

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Page 1: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 1

S4 Environmental DisturbancesRobert Schofield, U of O

John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO

Josh Dalrymple, SU

I. Pre-S4 “fixes”

II. Some S4 veto issues

III. Early coupling results from S4 PEM injections

Page 2: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 2

In E12, H2 AS_Q was dominated by FMY roll mode when excited by chiller

FMY roll mode peak in AS_Q increases when chiller matches frequency

drifting chiller seismic peak

? staging building chiller

Solution: resonant gain at FMY roll mode, seismic isolation of chiller.D.Q. flag for 10-100 Hz glitches produced by 16 Hz?

Office building chiller

LVEA

Page 3: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 3

10 Hz seismometer (etc.) peaks from RF card reader

original set up

after improving ground isolation of RF reader

Page 4: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 4

Transformers near test-masses contribute to 60 Hz AS_Q peak

AS_Q peak produced by transformer-sized magnetic field

Recommendation: keep transformers at least 15 feet away from chambers (annulus ion pumps?).

Page 5: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 5

Protecting sensitivity to the crab pulsarCrab GW frequency

Pump shut down

Pump left on

Coherence between LVEA seismic and H1, H2 AS_Q

Page 6: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 6

Up-conversion of low frequency seismic noise

seismic noise from distant excavation

night spectrum

excites stack modes in AS_Q

up-conversion reduces interferometer sensitivity

night spectrum

Page 7: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 7

Up-conversion experiments

Mechanical shaker at EX produces up-conversion in AS_Q

But matched injection into DARM and optical lever servo (pitch and yaw) does not produce up-conversion. This suggests that up-conversion is not produced in servo systems or by optic motion.

Page 8: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 8

Up-conversion of low frequency seismic transients

Produces large in-band event (and event triggers) coincident on both interferometers.

Small fast-traveling seismic transient

Page 9: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 9

time series of same transient, 0.7 to 2 Hz steep band-pass, seismometers at all stations

H2 AS_Q, 0.7 to 2 band-pass

H2 AS_Q, 70 to 200 Hz band-pass

Page 10: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 10

Coincident 1-3 Hz seismic, and 100-200 Hz AS_Q spikes

MY Seis Z 1-3 HzMZ Seis Z 1-3 HzH1 AS_Q 100-200 HzH2 AS_Q 100-200 Hz

This event does not produce up-conversion. However, this event does not show up in a sharper 0.7 to 2 Hz band.

Page 11: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 11

Why are airplanes signals so bursty in AS_Q?Continuous acoustic sources can produce 5x bursts in AS_Q.

Microphone signal (BP) from sound injection at REFL port

Band Pass on resulting acoustic peak in AS_Q

Bursts correspond with slight drops in arm power

Makes vetoing more complex!

Page 12: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 12

S4 LHO LVEA acoustic coupling from PEM injections

Page 13: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 13

S4 LHO out-station acoustic coupling

Page 14: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 14

S4 LLO corner and EY acoustic coupling

Page 15: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 15

S4 LHO EX, EY magnetic couplingWith predicted upper limits to displacement noise from coupling of ambient fields.

Page 16: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 16

PEM burst injection logs (also in elog)

LHO LLO

Page 17: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 17

SummaryI. Pre-S4 partial fixes

a. Wandering chiller seismic peak (D.Q. flag for 16 Hz?)b. 10 Hz from RFIDc. Transformers near test masses (ion pump supplies?)d. Crab protection (LHO out-stations, LLO?)

II. Some S4 Issues

a. Up-conversion of low frequency “continuous” seismic noiseb. Veto up-converting 0.7-2 Hz seismic transientsc. Continuous environmental sources can produce AS_Q bursts

III. Preliminary coupling results from S4 PEM injections

a. LHO LVEA ambient sound level generally less than 1/5 SRD above 60 Hz

b. LHO out-station ambient sound level generally less than 1/10 SRDc. 60 Hz peak in AS_Q may be dominated by direct coupling of ambient

magnetic fields

Page 18: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 18

Mechanical shaker near corner of chamber produces pitch, yaw and displacement motion as well as causing up-conversion in AS_Q.

Mechanical shaker beside chamber produces side motion, but little pitch, yaw or displacement, and does not produce up-conversion.

Page 19: LIGO-G050217-00-Z1 S4 Environmental Disturbances Robert Schofield, U of O John Worden, Richard McCarthy, Doug Cook, Hugh Radkins, LHO Josh Dalrymple, SU.

LIGO-G050217-00-Z 19