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Results of a Recent Instrument Response Test For Three Nodal Seismometers Dan Hollis (Sisprobe), Florent Brenguier (Sisprobe), Thomas Lecocq (Royal Observatory.

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Presentation on theme: "Results of a Recent Instrument Response Test For Three Nodal Seismometers Dan Hollis (Sisprobe), Florent Brenguier (Sisprobe), Thomas Lecocq (Royal Observatory."— Presentation transcript:

1 Results of a Recent Instrument Response Test For Three Nodal Seismometers
Dan Hollis (Sisprobe), Florent Brenguier (Sisprobe), Thomas Lecocq (Royal Observatory of Belguim), Larry Ortega (Western Oil Exploration), Jim Franklin (Dolomite Oil), Marianne Karplus (UTEP), Frank Vernon (SIO) SITS – 10/30/2018

2 2015 Instrument Test a receiver or node an array

3 2018 Nodal Instrument Test Test conducted at Piñon Flat Observatory
Broadband station BPH01 used as a control Deployment duration = 1 Day Instruments tested: Quantum 1C 5 Hz SmartSolo 1C 5 Hz Zland 3C 5 Hz a receiver or node an array

4 2018 Nodal Instrument Test Node Model Low-cut Filter Gain
Samples per Second Sensor Sensitivity Quantum N/A 24 dB1 250 “high sensitivity geophone” SmartSolo LCF = OUT DC Removal On 24 dB2 78.7 V/m/s Zland 36 dB 76.7 V/m/s a receiver or node an array Highest Gain Setting Highest Gain Setting. 3C SmartSolo allows up to 36 dB Gain (personal communication).

5 PSD for BPH01 Control Quiet station. 6-7 second seism stands out.
a receiver or node an array Quiet station second seism stands out. PSD with instrument response correction

6 PSD with instrument response correction
Quantum Results a receiver or node an array PSD with instrument response correction

7 PSD with instrument response correction
SmartSolo Results a receiver or node an array PSD with instrument response correction

8 PSD with instrument response correction
ZLand Results a receiver or node an array PSD with instrument response correction

9 PSDs with instrument response correction
All Results Quantum SmartSolo ZLand a receiver or node an array PSDs with instrument response correction

10 Earthquake Event a receiver or node an array

11 PSD without instrument response correction
Earthquake Event a receiver or node an array PSD without instrument response correction

12 12 hours Continuous Noise
a receiver or node an array

13 12 hours Continuous Noise
a receiver or node an array PSD without instrument response correction

14 Paths for recording lower frequencies with 5 Hz geophones?
a receiver or node an array Lower usable frequencies = greater depth imaging for ambient noise surface wave tomography. Higher sensitivity geophones (>78 V/m/s)? More gain options. Highest now is 36 dB. 42 dB? 72 dB? At what frequency is the geophone response too low to overcome amplifier and A/D noise?


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