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Identification and removal of glitches in GEO 600

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Not seen after work on the signal-recycling longitudinal error signal module around May. Broken switch from one error signal to another ... – PowerPoint PPT presentation

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Title: Identification and removal of glitches in GEO 600


1
Identification and removal of glitches in GEO 600
  • Joshua Smith and Stefan Hild for the
    GEO600 team GEO Meeting
    Glasgow, 11.10.06

2
Overview
After start of 24/7 S5 emphasis shifted toward
data quality Main glitch identification strategy
automatic characterization, mining this,
following up to find sources
  • Main Tools
  • GEO Summary pages
  • HACR
  • Coincident analysis
  • Noise projections
  • Now, KleineWelle
  • Glitch Families
  • The Owl
  • Sine-Gaussians
  • Dust
  • Laser frequency
  • MID slow FB
  • Magnetic field/mains

3
The Owl
  • Narrow line(s) with (sometimes) rapidly moving
    frequency
  • Is partially controllable, but not in
    well-understood way
  • Can cause poor data, glitches

4
Nevermore?
  • Not seen after work on the signal-recycling
    longitudinal error signal module around May
  • Broken switch from one error signal to another
  • This cant be the ultimate cause of the owl owl
    existed before this module

5
Owl and analysis
  • No good veto found yet
  • Could remove the areas of strongest owl presence
    by eye (cyan squares)

6
Sine-Gaussians
  • Few per day this summer. Source unknown
  • First look indicates some vetoed by null-stream
    (a combination of two GEO calibrated detector
    outputs that yields close to no GW signal)

7
Power glitches vs. dust
Particle count
Dark port DC power glitch count
Dark port DC power glitch count
Dark port DC power glitch count
Input port DC power glitch count
0 Time
m 180
8
Air Conditioning particle filters
140 (90)?20 factor 5-7
45 (25)?5 factor 5-9
(Particles/cu.ft)/1000
3 (2)?0.2 factor 10-15
A a
9
Dust made loudest glitches
Det. output BLRMS _at_ 170Hz
Time h
Time h
Before filter
After filter
10
Dealing with dust
  • Statistical vetoes look promising

11
Freq. Glitch Characteristics
0s
60s
  • Show up strongly in all frequency stabilization
    signals
  • Couple to H via frequency noise (MIC EP)

12
Removing MC2 glitches
2kHz
  • Traced origin to mode-cleaner 2 loop. Suspected
    saturation.
  • June 22nd Glitches drastically improved with 2x
    reduction of RF modulation depth (compensated by
    digital gain)
  • Surprise! Glitches return in July.
  • Found to be a switching comparator in
    modecleaner module, fixed glitches for good by
    changing threshold for this device

June
Freq. Hz
30d
0d
13
Vetoes for frequency noise glitches
  • Noise Projection vetoes (see Ajiths talk)
  • Null-stream veto (Martins talk)
  • Apply both, or in series?

14
Magnetic field glitches
H glitches
B glitches
Linear coupling, coherence
15
Magnetic field projection
  • B-field nearly limiting noise around 100Hz?
  • Coupling not yet understood
  • Checks magnetometer measures B-field, IFO
    back-coupling ruled out

16
Hourly mains glitches
  • Hourly series start
  • 24 secs after GPS hour
  • 10 secs after UTC hour

17
Mag./mains coinc. with H
Magnetometer central building 50coinc./8hrs
Mains monitor central building 30coinc./8hrs
Time-freq glitch maps
Frequency Hz
Frequency Hz
0
0
8
8
Time h
Time h
50
50
Time-shifted coincidence
0
0
1
1
-1
-1
Time shift s
Time shift s
18
Dealing with mains glitches
  • Could take out seconds 20 to 100 of every GPS
    hour.
  • Statistical veto
  • Filtering of Mains signal proposed for future

19
MID slow path glitches
  • Looks like a switch!

20
Coincident with mains glitches
  • Identify point of coupling already narrowed
  • Filtering mains may help elsewhere

21
Glitch rate at Start/end of lock
Glitches about equally distributed over the lock
stretches. No excess at the beginning or end (for
May)
22
HACR History Plots
May
June
July
August
23
Summary
  • Owl not seen after May 28
  • Sine-Gaussians seen mainly in May-June
  • Dust reduced drastically after May 22 by AC
    filtering
  • Laser frequency removed after Sept 7
  • MID slow FB traced to after digital feedback
    last week
  • Magnetic field/mains mains filtering a possible
    commissioning task
  • Current HACR glitch rate is about .035Hz
  • Often 5 times that in May

24
New KleineWelle G1 Triggers
  • Triggers online for S5 up till September
  • http//lancelot.mit.edu/cadonati/S5/online/Kleine
    Welle/
  • Thanks to
  • Laura Candonati, Lindy Blackburn for trigger
    generation, summary pages
  • Chris messenger for segment list generation

25
END
26
Frequency stabilization
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