Recent ground vibration measurements at CERN (Surface and underground)
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1 Recent ground vibration measurements at CERN (Surface and underground) Comparison with other measurements and overview methods K.Artoos, M. Guinchard 16 th October 2008, CLIC workshop
2 Contents : Overview references Ground Vibration measurements CERN measurements in LHC tunnel + surface Power Spectrum Density Integrated RMS + RMS histogram Coherence Conclusions More information: y
3 list of references (> # 60) Methods: V. Shiltsev, A. Sery et al., now INP S. Takeda et al. KEK 1994-now + other Japanese institutes References ground vibration measurements Available on new website stability/ground%20vibration%20studies.htm Absolute measurements : Seismometers, accelerometers, tilt gauges This talk Relative measurements : WPS, HLS, LASER Closed Orbit Distortion measurements Modified SM-3KV 8E4 Vs/m Hz STS-2 2*750 Vs/m120s- 50 Hz tilt meter, HLS 12 bit ADC 16 bit ADC 64 averages, blocks 1 minute at 1 khz Synchronisation: Electrical start trigger (~ ms) Synchronisation LON Network R. Amirikas, A. CMG-3TD, CMG-6TD, 24 1 minute blocks, GPS UTC time Bertolini et al. DESY Digital 24 bit, 360,60s - 80 Hz 2*750Vs/m 200 Hz down sampling bit minimum 15 minutes averaging USGS, CEA,... Specialised Geological survey CLIC, NSLS II, DIAMOND, XFEL,...
4 Set-up measurements at CERN : Guralp CMG 40T x,y,z 2*800Vs/m 1 km of optical Parameters fibre for synchronisation + Sampling rate 2 Muller-BBM timing 256 Hz MKII Analyzers and ddata Transfer Block duration 64 s Average Lin 50 Overlap 66.7 % 30 s -50 Hz ENDEVCO 86 PCB 393B31 Special credits to B. Bolzon, A. Jeremy! 24 bit on 100 mv Low ADC noise
5 Synchronisation Phase error < 0.01 deg
6 Measurements LHC DCUM 1000 ~ 80 m under ground LHC systems in operation, night time Floor building 180 Building 180 Surface No technical systems in operation, night time Measurements Combiner ring CTF 3 Measurements Combiner ring CTF 3 Some technical systems in operation, day time
7 Power Spectrum Density Guralp Endevco m/s m/s^2 2 (1 σ ( f )) DSP DSP σ 1 2 Noise (error) estimation by corrected difference 40 Hz
8 Power Spectrum Density: LHC Tunnel Vertical Technical gallery ATLAS ATL law
9 Power Spectral Density
10 Power Spectral Density A. Sery et al S. Takeda et al STS-2
11 k 2 Integrated R.M.S. LHC Tunnel RMSint ( k) = DSP( k). Δf g k 1 1 nm
12 Integrated R.M.S. 1nm
13 1 nm KEK 2008 A. Sery et al Hz 1 nm 1 nm 50 Hz
14 Example influence ventilation CLEX
15 Averaging, window, histogram, color map 50 averages of 64 sec blocks with 66.7% overlap: To have a good frequency resolution + definition of PSD To see something within the noise But: it s an average view Histogram Baklakov, Shiltsev et al. Fermilab 1997 R.Amirikas, A. Bertolini DESY 2005
16 Color map
17 Color map
18 Coherence measurements Guralp Regression and interpolation analyser software PAK
19 Coherence measurements LHC tunnel 10m 7m 6m 0
20 Coherence measurements Surface Building 180
21 What can influence coherence measurements? Phase shift Amplitude? Low signal to noise ratio micro seismic
22 Joints between concrete modules S. Takeda et al. 1996
23 Coherence: Comparison other measurements SM-3KV A. Sery, Coosemans 1994 LEP
24 Coherence: Comparison other measurements DESY
25 Conclusions Ground vibration level between 1 and 10 nm average integrated RMS at 1 Hz seems possible. Possible vibration sources like water cooling and ventilation should be carefully designed. Support or objects can amplify the ground vibration levels The ground vibration level can be increased by the resonance of a support or object For frequencies > 1Hz, coherence drops over a short distance It is possible to measure (averaged) nanometre displacements with seismometers but some characterisation of devices and analysis methods is still needed. S i i h b i l i i Seismometers with better signal to noise ratio are needed for active control purposes.
26 Spares
27 m/s 500E-9 Channel Guralp_01_EW Throughput Channel Guralp_01_NS Throughput Channel Guralp_01_V Throughput 400E-9 m/s 500E-9 Channel Guralp_02_V Throughput Channel Guralp_02_NS Throughput Channel Guralp_02_EW Throughput 400E-9 300E-9 300E-9 200E-9 200E-9 100E-9 100E-9 0E+0 0E+0-100E-9-100E-9-200E-9-200E-9-300E-9-300E-9-400E-9-400E-9-500E-9-500E s s
GROUND MOTION IN THE INTERACTION. ensured that the final focus quadrupoles on both. rms amplitudes higher than some fraction of the
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