Projects Stanford Micro Structures & Sensors Lab



Geophone Research

Isometric and Cross-sectional View of Geophone

Figure 1: An isometric and cross-sectional view of a geophone


Summary

Geophones are highly sensitive ground motion transducers that have been used by seismologists and geophysicists for decades. Figure 1 shows both an isometric and cross-sectional view of a geophone, which uses the motion of a spring supported coil in the field of a permanent magnet to generate an output signal. A typical geophone, such as the OYO Geospace GS-11D used in many of our group's measurements, costs $50, has a resonant frequency of 4.5 Hz, a proof mass of 23 grams, and a peak sensitivity of 20 V/g. The conventional geophone's ratio of cost to performance, including noise, linearity and dynamic range, is unmatched by modern, micromachined accelerometers.

However, a geophone is typically only used for high frequency (4Hz-400Hz) seismology experiments because its resolution degrades at low frequency. The poor low frequency (10 mHz-1Hz) performance arises because the output is proportional to the velocity of the proof mass, in this case the cylinder and coil assembly. We have been investigating methods to improve the performance of a geophone through feedback and position sensing in various combinations.

The sensitivity of a geophone as a function of frequency can be altered by feeding back the conventional output. This will not improve the resolution, but will amplify low frequency signals. However, the resolution can be improved by measuring proof mass position. Currently, we are been building and testing capacitive geophones to demonstrate an affordable, broadband seismometer.


Recent Publications

This section contains the presentations we have given on our geophone research. As our work has progressed, we have made some changes in our approach. Therefore, consult the most recent publications for our most accurate information. The earlier work is here as an archive and has not been changed to reflect new results.

Seismological Society of America 1999 Annual Meeting
"An Affordable Broadband Seismometer:The Capacitive Geophone"
At this meeting, we presented results on the performance of a capacitive geophone based on the OYO Geospace GS-11D 4.5 Hz vertical geophone. A new circuit is used, which has been fabricated on a printed circuit board(PCB). The acceleration sensitivity is 63 V/g from 83 seconds to 50 Hz, while the velocity output has a sensitivity of 6.3 V/m/s from 45 sec to 50 Hz. The sensitivity has been verified experimentally down to .2 Hz and up to the high frequency rolloff. Resolution measurements have been taken, but they are limited by the ambient noise present during the measurement. Nevertheless, it sets an upper limit on the resolution.
Poster 5/4/99 Slides in Powerpoint(Mac 4.0) format
Slides in PDF format
Circuit Schematics 5/4/99 Part I,Position Measurement circuit, in PDF format
Part II,Controller circuit, in PDF format

ASME International Congress Winter '98
"Improving the Performance of a Geophone through
Capacitive Position Sensing and Feedback"
At this meeting, we presented preliminary results on the performance of a capacitive geophone based on the Mark Products L-40 40 Hz geophone. While the results demonstrate the principle, more work needs to be done. The talk (not the manuscript) is the first presentation where we measure the phase of the signal on the center electrode, rather than the magnitude.
Talk 11/20/98 Slides & notes in Powerpoint(Mac 4.0) format
Slides in PDF format
Notes in PDF format
Manuscript 7/7/98 Manuscript in PDF format
Manuscript in Postscript format

Review of Scientific Instruments
"Technique for measurement of the noise of a sensor
in the presence of large background signals"
This paper describes a method to measure the resolution of a sensor in the presence of large background signals. We use this technique to measure the resolution of the seismometers we build. If our lab were a quiet environment, we would just operate one instrument without exciting it to measure the sensor's noise. However, we are trying to build sensors whose resolution is better than 100 ng/rootHz. The background seismic signal in our lab is typically over 1 micro-g/rootHz. Therefore, when operating one of our sensors without applying an input, we measure the background seismic signal, not the sensor's noise. We avoid this problem, as described in the paper, by operating two identical sensors side-by-side and measuring the fraction of the output that is incoherent. Since the sensors are excited by the same signal, the small amount of incoherence is caused by sensor noise.
Manuscript 7/98 Manuscript in PDF format on RSI website

AGU Spring '98
"Improved Low Frequency Performance of a Geophone"
This is the first presentation we gave on capacitive geophones. It presents background information, the concept of a capacitive geophone, and a theoretical analysis of the sensitivity and resolution of a capacitive geophone. At this point we were measuring the magnitude of the signal of the center electrode (see ASME Winter'98 talk) rather than correctly measuring the phase. This poster does not present experimental measurements of a capacitive geophone.
Poster 5/28/98 Slides & notes in Powerpoint(Mac 4.0) format
Slides & notes in PDF format



Aaron Barzilai barzilai@leland.stanford.edu 4/30/99