` Yuma-2 Seismometer

Yuma-2 Force Balance Vertical (FBV)

Seismometer Project

Click here for the latest real-time seismic measurements from Bend, OR, USA

  Yuma-2  Yuma-2

This page documents my experience building and operating a very sensitive amateur seismometer, called Yuma-2. This instrument was designed by Dave Nelson and Brett Nordgren, and is the second in a series of three designs. First came Inyo, then Yuma, and most recently Napa. At the time I started building, Napa was still experimental, and Yuma was recommended as the most mature design, and the best one to begin with. These are extraordinary instruments, for their capabilities and their well thought out mechanical and electrical design. I did not know much about seismometers or seismology when I began this journey, and I've been throughly impressed with the work and results that this small community of developers has achieved.

I wanted a project that was substantial, challenging, required high precision, and would allow me to learn some machining skills. I wanted to build something that measures some aspect of the world around us, sensing things that go unnoticed by most people. The Yuma turned out to be a perfect choice.


The instrument itself is relatively small, fitting in a case that is about 23 x 20 x 14 cm. It comprises a horizontal boom suspended by a leaf spring, with a differential-capacitive position sensor and voice-coil actuator. Trim weights are adjusted to set the rest position of the boom assembly at the midpoint of travel, and to align the sensitive axis with the vertical. Any disturbance in the boom position is sensed and amplified. This signal is fed into an analog PID (proportional-integral-differential) control circuit where it generates a control signal to drive the voice coil actuator to oppose the disturbance. This feedback loop keeps the boom nearly perfectly centered at all times. Careful filtering is done to tailor the frequency response of the system. The high gain of the feedback loop compensates for the natural limitations of the mechanical system. The result is an instrument that can detect ground velocity with low noise over a wide range of frequencies, from a few milliHertz to over 30 Hz. 

Sensitivity is impressive. Not having had much exposure to seismology or the instruments that professionals use, I couldn't believe the numbers when I first heard them. Properly installed at a good site, this instrument can detection motions of a few tens of nanometers/sec. Coming from the world of electronics where cutting-edge integrated circuits are fabricated at similar nanometer scales, and considering the cost and complexity of the instruments that operate at these scales, I was amazed that an amatuer could build an instrument with such sensitivity.

This level of sensitivity demands attention to detail. All manner of secondary effects come into play as sources of noise which obscure these slight movements. With the seismometer out in the open, even in a quiet room with still air, imperceptable air currents buffet the boom causing it to move up and down at a microscopic scale.

As we know, the atmospheric pressure around us changes slightly. Pressure and temperature changes cause air density to change. The aluminum and brass that comprise the boom have some amount of boyuancy in air.  Of course, its not enough for them to float off the table, but it is enough for them to weigh slightly less in dense air than they do in thin air. This difference is detectable by the instrument. So air pressure and humidity must be stabilized. The seismometer is mounted inside of an airtight case. But, the changing atmospheric pressure causes the walls of the case to warp ever so slightly. If care is not taken, some of this force would be transferred to the base plate of the instrument, causing it to warp ever so slightly. With the sensitivity of this instrument, such minor deviations would show up in the data. So Dave and Brett designed an ingeneous and effective implementation of a 'warpless' base to avoid this problem.

The leaf spring, made of 17-7 stainless alloy, was specially heat treated (precipitation hardended) to stabilize it over the long term. Without that step, small pops could show up in the data, as various metallic domains in the spring relaxed under the tension.

Air itself is a viscous fluid, and it will oppose the motion of a plate, like that of the boom against the capacitive position sensor. So a network of holes were designed into the PCB to allow that air an escape route when the boom moves up and down a few microns.

The electronics are designed to be very low-noise. Chosing the best components for these designs was not a simple matter of looking at datasheet specs. The designers simulated, tested, and characterized these circuits for the specific regime where they would be operating, to find those op-amps, capacitors, and other components that were best suited for the task at hand. Flicker-noise is a common problem in low-frequency circuits, and the chosen amplifiers have very low 1/f noise at the frequencies of interest, without having significant temperature effects, or input bias currents, or offset drift. Film capacitors were chosen in the signal processing chain for high linearity, absence of piezoelectric effects, and minimal capcitance change with applied bias. After PCB assembly, thorough cleaning of flux residue ensures no leakage currents that might increase over time and degrade the performance of high-impedance circuits.

There are literally dozens of small effects that must be understood by the designers and carefully addressed in the design. It's clear that these guys have an amazing amount of practical hands on experience and knowledge in this area. And they've been a pleasure to work with.

I built Yuma-2 mechanical revision 4.3, electrical revision 4.0. Click here for:
Many of the documents and information on this site were taken from Brett's website, and others.

Here's how the Yuma compares to several professional instruments:

Guralp CMG3
Velocity broadband
Velocity broadbandVelocity very broadband
Velocity very broadband Velocity very broadband
Flat response
20 mHz - 30 Hz
33 mHz - 50 Hz2.7 mHz - 10 Hz
8.3 mHz - 50 Hz
10 mHz - 50 Hz
Generator constant
1344 Vs/m
1500 Vs/m2 x 1200 Vs/m
2 x 750 Vs/m
2 x 750 Vs/m
Operational range
+/- 15 mm/s
+/- 5 mm/s+/- 8 mm/s
+/- 13 mm/s
+/- 13 mm/s
23 x 20 x 14 cm
22 x 18 cm12 x 17 x 18 cm
23 x 26 cm
17 x 37 cm
11 kg4 kg 13 kg
14 kg
~0.5 W (not incl ADC)
0.4 W3.5 W
0.8 W
0.75 W

Refer to some of Brett's documents for details on the theory of operation:

Vertical Geometry Seisomometers
Use of Feedback in Seismic Sensors
Good analysis of closed loop seismometer
Astatic Geometries
Inyo Circuit Description

An excellent free text on seismology is the New Manual of Seismological Observatory Practice, consisting of chapters, datasheets, downloadable programs, and more.


I purchased from Webtronics, Larry Cochrane's PSN-ADC24, a four channel 24-bit low noise ADC board with USB/Serial interface. This is a good board at a reasonable price, and it's specifically designed for seismology applications.  It integrates easily with two pieces of seismology software, widely used by the community, WinSDR and WinQuake.

ADC24  ADC24 block diagram

I'm using board version 1.5. Larry kindly configured the channels with different voltage dividers that I requested:
10V input  2.5V input

The CS5532 from Cirrus Logic has an internal chopper-stabilized PGA with good noise specs, as low as 6nV/rtHz.
Voltage reference is the 2.5V LT1019CN8-2.5 (3ppm/C stability, 0.05% initial accuracy)

The ADC bipolar full scale range is 2.5V (-VREF to +VREF) when gain=1. (I'm assuming Larry sets the VFS bit = 1)
On the board, the ADC is biased at midrange, so AIN inputs are 2.5Vcm +/- 2.5Vdiff: AIN+ = 2.5 + 1.25, AIN- = 2.5 - 1.25

ADC input voltage
ADC counts
-VREF / gain
0x800000 (-8388608)
VREF / gain
0x7FFFFF (8388607)

For Channels 1, 2, 3. At gain > 1 the internal PGA is enabled, reducing input current to 1.2 nA. Therefore gain = 2 mode is used.
Note: in the table below, DIV = 17.0, the resistor divider ratio

ADC Gain
ADC bipolar
full scale range
(AIN+ - AIN-)
Channel full scale
differential voltage range
 (IN+ - IN-)
ADC counts
'Amp Gain'

2.500 V 42.5 V (IN+ - IN-) / DIV / 2.5 * 2^23
5.07 uV / LSB
1.250 V 21.25 V (IN+ - IN-) / DIV / 1.25 * 2^23 2.53 uV / LSB
625 mV 10.625 V (IN+ - IN-) / DIV / 0.625 * 2^23 1.27 uV / LSB
312.5 mV 5.313 V (IN+ - IN-) / DIV / 0.3125 * 2^23 633 nV / LSB
156.3 mV 2.657 V (IN+ - IN-) / DIV / 0.15625 * 2^23 317 nV / LSB
78.13 mV 1.328 V (IN+ - IN-) / DIV / 0.078125 * 2^23 158 nV /LSB
39.01 mV 664 mV (IN+ - IN-) / DIV / 0.0390625 * 2^23 79.1 nV / LSB

Note: WinSDR doesn't seem to take the ADC gain setting into account when displaying the data in units of "ADC volts". So divide by gain to get the correct value. See this spreadsheet for my measurements.

Before connecting to the instrument, I made some noise and frequency response measurements of the ADC.

The digital filter inside the ADC has a sinc5 rolloff. This means you need to sample significantly faster than Nyquist to minimize attenuation of high frequencies. Since I'd like a flat measurement bandwidth of 20 Hz, I chose to sample at 200 sps, the highest supported rate in WinSDR. (There are a couple downsides to this: more noise due to less averaging, and the loss of the 60 Hz notch filter, so AC mains noise might become a problem.)  An alternative would be a digital equalization filter to compensate for the sinc rolloff, while running at a lower sample rate.

Measured attenuation
1 Hz
0 dB
2.5 Hz
0 dB
5 Hz
0.04 dB
10 Hz
0.08 dB
20 Hz
0.22 dB
Noise was measured with inputs shorted. These numbers are worse than the data sheet spec by 1-2 bits. But I don't really trust the datasheet. There are also some funny noise distributions at 50 and 200 SPS.
Note: noise free bits = ln(Full-scale range / Vpp noise) / ln(2):

CH4. Divider=1, Gain=1, 0.1 Hz HP 2 pole filter, 120 second window.

Samples / sec
DN p-p noise
uVpp noise
Noise Free bits
2.7 uVpp
2.7 uVpp
4.5 uVpp
4.7 uVpp
37 uVpp

CH2. Divider=17, Gain=2, 0.1 Hz HP 2 pole filter, 120 second window.

Samples / sec
DN p-p noise
uVpp noise
Noise Free bits
18 uVpp
25 uVpp
1846 uVpp
53 uVpp
68 uVpp
303 uVpp

See the "Results" section below for a PSD of the ADC data with inputs shorted, and compared to Yuma-2 outputs.

Filtering in WinSDR is an ongoing experiment for me, but currently I am running only high pass filters on the raw data:
In WinQuake I have played with several filtering options, including the period-extending inverse filter. I still have a lot to learn about best practices here.
For distant quakes this filter does reasonably well:

WinSDR Configuration

Click on the images below for full size. Configuration of WinSDR, low gain channel:

High gain channel:

System settings:

Larry has generously provided a utility called drf2txt that will dump the data from the WinSDR daily record files to plain text and CSV format for further processing.  I find this useful to further process the data with some python scripts.

WinSDR has a nice feature, a TCP server on port 16064, that can be used to receive the raw ADC measurements.  I'd like to use this to tap the data stream so I can play around with the live data, without interrupting the data collection and graphing in WinSDR.


To ensure we're making accurate meaurements, it's necessary to make various measurements so we can properly calibrate the output of the instrument.
The FBV is a velocity broadband seismometer with this architecture:
VBB diagram
The instrument parameters are summarized here.  See the sections below for details on how these were determined. The ADC numbers assume 200 SPS, and gain=2, and no filtering.

Velocity response flat from 0.02 Hz to 30 Hz
Output channels high gain, low gain, internal temperature, and centering force
Coil Forcing Constant, Gn 9.3 Newtons / Ampere
Coil / Magnet
41.0 ohms, 542 turns 34AWG / N45 magnet
Generator Constant (Ag) 336.2 Volts / meter / sec
Ag High gain output, (Ag HI) 33,599 Volts / meter / sec
Ag Low gain output, (Ag LOW diff) 1,344 Volts / meter / sec
Boom free period 2.3 seconds
Boom moment, M0 87.5 g

ADC board input impedance
38 kOhm
ADC divider ratio 17.0
ADC reference voltage 2.5V
ADC input full scale range, gain=2
+/- 1.25V (-VREF/2 to +VREF/2), Vcm = 2.5V
ADC board full scale range, gain=2
+/- 10.625 V (for -VREF/2 to +VREF/2)
ADC Quantization 2.53 uV/Count (24 bits)
ADC gain flatness
-0.2 dB at 20 Hz
Quantization (HI) 0.0753 nm/s/count. (unfiltered ADC noise: 9 nm/sec pp)
Quantization (LOW diff) 1.88 nm/s/count. (unfiltered ADC noise: 225 nm/sec pp)
Clipping level (HI)
632 um/s
Clipping level (LOW diff) 1.58 cm/s

Measure critical component values

Measured by U1272A @ 22.2C
30.452 uF
30.436 uF
not measured. nominally 1 uF
41.0 ohms

Forcing coil constant Gn

The coil constant, Gn, was measured two ways. Unfortunately there's some discrepancy in the two results, but I think this is due to my reconfiguration of the magnet and pole piece, and some slight misalignments.

First, the magnet/coil assembly was tested separately, by placing magnet assembly on a scale, suspending the coil above from an aluminum bar. Inject known current (+/-50mA) into coil and measure change in weight.

Gn =  Δ Weight * 9.81 / current
Less than +/- 3mA, coil constant: 10.5 +/- 1.0 N/A
From +/- 50 mA, coil constant: 9.62 +/- 0.48 N/A.
(These values had been measured with a slight misalignment of the coil.)

542 turns, AWG34, N45 magnet, Rc=43.7 ohms.
Gn = 9.6 +/- 0.5 N/A

GN can be measured with the instrument assembled and operating normally. First record the coil resistance, Rc, and the measured value of Ri. Attach an accurate voltmeter to the"CENT FORCE" output, pin 6, and turn on the seismometer. Balance the boom if necessary and after it stabilizes, record the voltage, VCF . Then place a 500mg weight on the top of the boom at the same distance from the pivot as the center of the coil. If necessary, any approximately 500mg non-magnetic object whose weight is accurately known, such as a #6 brass washer, may be used instead of a 500mg standard weight. After the output on pin 6 settles, record the new voltage. The coil constant Gn = W/ δVCF * 0.00981* (Ri+Rc) N/A, where W is the test weight value in grams..

Using the second method, on a fully assembled instrument, remeasure Gn by using CF output and known mass on boom, at coil mount:

Ri = 14.985K. Rc = 41.0 ohms.
Measured CF = -0.5622 V
Add 500mg calibration weight.  Allow to stabilize 5 minus. CF= -8.513V

delta V = 7.9508 V
delta I = 7.9508 V / (14985+41 ohms) = 5.2914e-4 Amps
delta F = 500e-3/1000 * 9.81 = 4.905e-3 N
Gn = F / I = 4.905e-3 N / 5.2914e-4 A

Gn = 9.27 N/A

Boom mass M0, M1

First, the instrument may be assembled without the spring and the effective boom weight measured by means of a sensitive scale, arranged to support the beam so that it is level, at a point which is the same distance from the pivot as the center of the coil/magnet. That gives M0. When using particularly flexible (Kapton) flexures, watch to be sure that without the spring, they aren't flexing downward too much during the measurement.

Spring: 4.7g
Boom w/o spring or weights (including vertical brass threaded rod): 165.1g
Boom with weights: 210.3g
Hanging support: 10.5g + 0.5g nut = 11.0 g
Measured weight at nominal position: 98.5g

Net boom mass, M0 = 87.5g
M1 is difficult to measure. Estimated 110 g

Free period

Free period was measured by disconnecting the coil, selecting GAIN=1 by removing JP1, and measuring POSN_ERR output while generating an impulse with a canner air duster. This was repeated several times. The measurement was made 7.5 seconds after the impulse to try to capture the small signal reponse. Period was measured on the scope to be 2.3 +/- 0.1 sec. An FFT of the data indicated a period of 2.26 sec. Zeta was determined to be 0.15, by fitting the data to a damped harmonic oscillator.

Free period   Free period

Sensor gain, Rsensor

To measure the sensor gain, remove jumpers JP1 and JP2 and unplug the connection to the forcing coil. Arrange for the boom to seek its upper stop, either by installing and adjusting the spring or by means of an external spring such as a rubber band gently lifting the boom. Mount a micrometer or micrometer head to press down on the boom at the same distance from the pivot as the center of the coil. Mount the micrometer so that it can move the boom over its vertical range. Starting with the boom approximately centered, connect a meter to the 'POS ERR' output, pin 7 and turn on the electronics. After the voltage stabilizes, using the micrometer, move the boom in steps in both directions from center over about half its range, approximately 0.4mm or 0.015", while recording the micrometer readings and corresponding output voltages. The slope of the data curve at its zero-volt point (change in voltage/change in position in mm) should be approximately 12.5V/mm, which, multiplied by R6/R29 (nominally 1/10), will give the value of rsensor

Since I didn't have a micrometer head, I chose to do this measurement on my mill. Rubber bands provided upward tension on the boom. A pointed tip in the chuck pressed down on the boom at the coil mount screw. The Z-axis DRO measured position as I recorded POSN_ERR output voltage.

measuring rsensor

sensor measurement sensor mean

Notice how the zero crossing is not in the symmetrical part of the curve. I suspect the boom is not planar with the PCB at zero position, possibly due to flexture sag or machining errors.  The flexture gap was set to 10 mil with a feeler gauge. Accounting for the -10X gain of the POSN_ERR output stage:

Rsensor:     1118 V/m

Centering Force

The centering force output was measured to be delta -7.951V with an additional 500 mg calibration weight on the boom, at the coil mount point.
CF = -7.9508/500e-6 = 15902 V/kg

Centering Force sensitivity = -15.9 Volt / gram, where negative means additional force supplied by the coil.


You really can use two balance weights, one horizontal and one vertical, though just one can be used if you accept a somewhat more complicated adjustment procedure. A properly balanced boom will have its center of mass lying in the same plane as the pivots. This means that its sensitivity to horizontal motion is minimized; or stated another way, its sensitive axis is close to vertical. Then the boom mass and the horizontal location of its COM will need to balance the spring when its length has been adjusted to get 3-seconds or so, free period. The spring adjustment sets the free period; the mass is just trimmed horizontally for balance. If you used two balance weights, you could make them adjust the x and y coordinates of the COM somewhat independently. Initially the COM will be located below the level of the pivots, mainly because the coil mass is fairly significant and is below the pivot plane. To balance, with the spring removed, but everything else on the boom in place, hang the boom coil down. If the pivot gap isn't too much over 0.010", the flexures should work fine in compression. The vertical trim weights are adjusted until the boom hangs straight down. Horizontal balancing is done at the time you are first adjusting the free period. Fine trimming can be done with a thumb nut or two on an horizontal brass screw, mounted as you observed below. With minimal horizontal trim weight, start shortening the spring until the boom balances and check the oscillation period. It will be less than 3 sec. Shorten the spring by a couple of thousandths (of an inch), temporarily add a bit of weight near the coil for balance (small brass washer or nut?), and check the period. Shorten more and rebalance, etc., etc. When you get up to something around 3 seconds, you can permanently attach equivalent weights (on the coil screw?) and then make final balance adjustments with the horizontal thumb screw(s).

Download the balancing spreadsheet: Tilt_test_357.xls

The vertical axis of the instrument is aligned within 0.26 deg of true. Horizontal sensitivity is 0.44% of vertical sensitivity. This is a pretty good result.

Since the sensitivity angle is negative, the vertical trim weight is slightly too low.
The centering force error is -22 milligrams, so the horizontal trim weight is slightly too close to the pivot.
tilt test alignment
Confirmed polarity of coil matches schematic - positive voltage moves boom upwards. The loop polarity spreadsheet has been recently updated to account for the Yuma2 circuitry.

Instrument Generator Constants 

Computed from Loop8Y.xls:
Ag 336.20 V/m/s At feedback Loop output
A hi + 33,599 V/m/s OUT HI +  
A low + 671.98 V/m/s OUT LOW +
A low - -671.98 V/m/s OUT LOW -
A low (total) 1,344 V/m/s (Out LOW +) - (OUT LOW -) 

As you can see later, this matches the SPICE simulation within 2%.

Poles and zeros

Transfer function computation, using Loop8Y:

Corner Frequency
-8.433e-4 +/- 0.08498 0.02 Hz
-209.7 (appx)
33.4 Hz
-1000 + 0j  159 Hz
-1002632 + 0j 160 KHz
LO -
-1002632 + 0j 
160 KHz
LO +
-100263 + 0j    
16.0 KHz
Note: The pole at 33.4 Hz is estimated based on LTSpice simulation.

Corner Frequency
0 + 0j 0 Hz
-4.167e-6 + 0j 0.7 uHz

The instrument response to ground velocity is calculated using Brett's Loop8Y.xls spreadsheet, using measured values for electrical and mechanical parameters, and the Rev 4.0 schematic. M1 has been estimated at 155 g.
Yuma-2 response
system responses
Loop gain measurements

Using the loop test board, I measured the gain and phase of the feedback loop.  The loop was broken and a signal generator was inserted to inject a signal into the fedback loop. By measuring voltage and phase shift, several things about the feedback loop are characterized. The crossover frequency, where loop gain drops to unity, and phase margin at the crossover frequency are important metrics to assess loop stability and compare against expected values. 

Surprisingly, the crossover frequency was much higher than expected.  It was measured at 58 Hz, with 48 degrees phase margin. This is sufficient for stability, but a crossover frequency closer to 30 Hz was expected based on the Loop8 spreadsheet.

I ran some Spice simulations to investigate the discrepancy. See the Simulation section below for details.
loop gain
Temperature sensitivity

Over 5 days, the Centering Force output (inverted), was compared against the internal temperature sensor, over a narrow range of temperatures. The sensor is mounted on the PCB, while the CF is primarily affected by the temperature of the spring. CF is a -1X output from the integrator, so the integrator has a +31 mV / C coefficient. This is exactly one tenth the value measured by another builder. I'm not sure what the source of this discrepancy is. 
Using the coil force constant, and the value of Ri, this represents a force difference of 2 mg / C.  Using M0 measured above, this is 23.1 ppm / C.
dF/dt = 0.267 V/degC / 14985 ohms * 9.6 N/A / (0.0875 kg * 9.81m/s^2) * 1e6 = 206 ppm/degC

The spring constant is expected be about 250ppm/C.

(On the plot there is an inadvertent gap of several hours when the data recording was interrupted.)
cf vs temp cf vs temp


Starting with Brett's SPICE model of the mechanicals and control loop, I added the output amplifiers of the circuit and tweaked the parameters to match my Yuma, as measured.  SPICE is typically used as an electrical simulation tool, but mechanical systems can be modeled as well, since they share the same underlying physical equations.  In this case the spring-mass-damper and forcing coil were modeled using the 'Force-Voltage' analogy for translational mechanical systems.  In SI units:

Force (N) = Voltage (Volts)
Velocity (m/s) = Current (Amps)
Mass (Kg) = Inductance (Henries)
Damping (N/m/s) = Resistance (Ohms)
Compliance (m/N) = Capacitance (Farads)
Displacement (m) = Charge (Coulombs)

LTSpice Schematic

If you want to simulate in LTSpice, here's the schematic file and the AD706 model.

It's nice to have a complete model of the electromechanical system that be be simulated in its entirety. A few comments about the model:

Displacement sensor is assumed to be linear.
Spring TempCo not included.
Simulations tested: transient, AC, noise.

Simulation results match the Loop8 spreadsheet closely. Low gain channel is determined to be 1389 V/m/s. High gain channel is 34320 V/m/s. This is within about 2% agreement.  Simulation predicts flat velocity response from 21 mHz to 33 Hz.  Noise at 20 mHz is predicted to be -153 dB m2/s2/Hz.  At that frequency, the largest contribution to noise is the Johnson noise of the coil resistance (7 uV/√Hz, referred to output.)

The coil noise is still the subject of some uncertainty. It appears the real instrument has lower noise than the simulations suggest. Brett is using a custom op-amp noise model that has noise more closely resembling real measurements, at or below the NLNM noise floor.  The AD706 macro-model simulates worst case datasheet parameters, but for noise the datasheet only provides typical values.

Simulated gain     Simulated gain

To investigate the discrepancies found during loop gain testing, I tried a few things to try to make the Spice simulation fit the measured data.

I made a separate circuit model to simulate the position sensor in isolation. The original Yuma spice circuit had a pole in the position sensor circuit that was slightly off, compared to the simulation results of the LTC1043 circuit. This affected the phase margin of the loop.  The LTC1043 is a switched capacitor circuit and the model from Linear does not seem to be capable of AC analysis. So I ran a transient analysis and fit the step response of the circuit to a single-pole RC filter. I used a voltage-variable capacitor model from here. The result was a response with a single pole at ~340 Hz. The sensitivity of this circuit is quite amazing. For a +/- 10 micron displacement, it is measuring only half a picofarad of capacitance change! And typical boom movements are much less than that.

LTSpice schematic and capacitor library and symbol.

LTC1043 circuit
LTC1043 output

Next, I played with the M1 mass to shift the crossover frequency to the right place (decreased it to M0 value).  I played around with the leakage inductance of the coil to get the right shape to the gain curve near 100 Hz. I adjusted the Rsensor gain to correct the overall gain (increased it by 24%). After this, I had a circuit model that matched the measured data more closely.  But I have some doubt whether these adjustments reflect reality. They don't agree with my earlier measurements of the sensor gain, and the mass change doesn't make sense to me.

Closest match was found to be: Rsensor = 1380 V/m, M1 = 87.5g, Gn=9.27 N/A, leakage inductance = 3 mH.  At Fc=58 Hz, the gain of the simulated circuit is -0.8 dB, and the phase margin is 48 deg.

LTSpice schematic.

LTSpice Schematic

  loop gain sim


As mentioned earlier, care must be taken to install the instrument properly for best results. Based on recommendations by Brett, Dave, and other members on the mailing list, I've chosen a few things for my particular situation. Living in town, in the Bay Area, I do not have a low background-noise site. Traffic, trains, low-flying aircraft, neighbors, and household equipment all contribute significant seismic noise, which this instrument easily picks up.

Currently my Yuma is set on a granite tile, which is resting on the concrete floor of my garage. The legs are leveled, based on earlier calibration. Small pieces of lead sheet are placed under the legs, and at three points between the granite and concrete to help stabilize the instrument and reduce noise from differential CTE of materials.

The instrument is connected to the ADC with a ribbon cable of approximately 18 inches. The cable is currently unshielded, but the adjacent grounds of the connector pinout provide some minor level of shielding. The cable is strain-relieved by wrapping it under the Yuma to avoid pulling on the side of the case.

An insulation wrap made from several layers of polar-fleece fabric surrounds the Hammond case, with cutouts for the legs. A thick styrafoam cooler, without the lid, is set upside down over the installation. A small weight on top keeps it secure. A future addition might be styrafoam insulation for the the ADC case, to keep any temperature-related drift to a minimum.

The ADC is connected over USB to a Raspberry Pi, running ser2net, a TCP/IP to serial port utility that supports RFC2217 for low-level remote control of the port. (See config here.) The Pi is connected over wired Ethernet to the home LAN, and a laptop is running WinSDR. I'm currently using Serial Port Redirector by Fabulatech to fake a local COM port for this remote setup. I might change to a freeware alternative, but so far none have proven reliable.


So, the big question is: how well does it work??

Bear in mind that I still have a lot to learn about proper filtering, installation optimizations, and noise mitigation techniques. But the results so far have been an eye-opening experience.

The first thing to note is the strong diurnal signature of cultural noise, all the man-made background that comes with living in a metropolitan area. My location is 2 blocks from the main throughfare in town, 1/3 mile to a commuter rail line, and 3/4 mile to the nearest expressway. Clearly this is not the ideal location for a seismic monitoring site.  Even so, I have to say I'm pleasantly surprised with the results.

In the Bay Area, small quakes are commonplace. Typically, we've been getting several per day less than M3.0 within 100 miles radius of my location. A normal person would likely never feel any of these. These small quakes are completely normal for the geology of the area. The Yuma picks these up easily, and depending on their strength and location they can be quite prominent in the data, or visible only after close examination.

Large distant quakes, called teleseismic events, are also within reach of the Yuma. Wikipedia states that modern (professional) seismic instruments can detect an M5.3 anywhere in the world. Having just started out with this, I'm just beginning to build up my dataset of distant quakes. However, a few days after installing the Yuma, I detected a very clear signature of a M6.2 event over 6000 miles away near the coast of Chile.

(Note that I had not properly calibrated the WinSDR settings so you can disregard the y-axis units. I am also just guessing at the locations of the P and S waves, but they are consistent with a quake at the specified distance.)

Chilean M6.2

Compare this to the same quake recorded at a college station in central CA:

A few days later, a nearby M2.9 occured a few miles away in the foothills near Cupertino. The strong signature is visible near the center of the chart.  Also on this chart is an M2.7 at 15:47 UTC and an M2.1 at 08:41 UTC.  The rest is mostly local noise.  Notice how the night (top) is much quieter than the day (bottom).


The farthest and faintest I've caught yet was a M5.6 South of Sumatra, about 9000 miles away. If my calibration factors are to be trusted, the measured motion was less than 250 nm/sec. This quake arrived at nighttime when it was quiet. (The markers for LQ and LR are inaccurate due to the wide variability in the speed of propagation of surface waves.)

M5.6 Sumatra

The damaging M7.8 in Nepal, including some aftershocks, came rumbing through over 3 hours.

M7.9 Nepal

Listen to the Nepal quake as a WAV file, filtered 0.01 Hz to 0.07 Hz and sped up many times.  One second of audio time is just over 1 hour of real time.

Here are a few distant quakes:

23:54    M5.1 in New Guinea
02:55    M4.7 in Alaska
09:08    M4.7 in Guatelama
10:30    M5.5 in New Guinea

high gain

Update 12/30/15: Here are animations of about 6 months of recordings from the low gain channel and high gain channel.

A good quake tracking site is http://earthquaketrack.com/recent

Interesting man-made sources that appear regularly are late-night freight trains, nighttime street sweepers, and large aircraft on approach to Moffett Field. There are a few more that I haven't identified yet. The trains are interesting because I can see them make their way up or down the penninsula by comparing my traces to those of another Yuma in Palo Alto, 9 miles away, run by Gary Lindgren. Larry Cochrane has seismometers running in Redwood City, about 15 miles from here.

A power spectral density plot compares the Yuma low gain output against the NLNM (New Low Noise Model) and NHNM (New High Noise Model) ground velocity. These represent worldwide background averages at professional stations. Each plot represents 7 hours worth of data at 30 sps. The data was not filtered. First plot is 7 hour of data at night, second is 7 hours of data during the day.

The shape of the data indicates that my Yuma really is picking up signals consistent with the natural background seismicity of the Earth.
In the plots below, the noise floor was calculated using a SPICE simulation of the actual circuitry (including Analog's model for the AD706).

psd vel psd vel
psd vel psd vel

I noticed that my noise floor measurements are different from what Brett computed, using his own custom noise model for the AD706, and slightly different component values from my Yuma.

psd vel psd vel

As a comparison, here is the noise spectrum with the ADC inputs shorted.  This was taken over a shorter time period, so the low frequencies are less accurate:

psd vel adc shorted inputs

Update 11/20/17: I should have included these coherence plots two years ago when I created them, but better late than never... The two-instrument Holcomb technique is a way to estimate instrument self noise, by comparing the signal received by two more-or-less identical instruments in the same location. (An even better technique is Sleeman self-noise measurement,which uses three instruments.)

Using Gary Oliaro's work as a guide, I wrote this python script to generate these plots, which estimate the coherence and self noise from my two Yumas. The dataset (122615_000000.txt) was taken during a 24 hour period that was relatively quiet, with no major earthquakes and only one small one. Since it was the Christmas holiday, only a single train was passing through. The data was collected with a 0.002 Hz single pole HP filter. At this time, Unit 2 had an incorrectly-wound coil (too many windings) with a higher force constant, so its gain is lower. Unit 2 was (unfortunately) installed 90 degrees rotated to Unit 1. For this reason they might have had different sensitivities to low-frequency ground tilt. Any horizontal axis sensitivity would have also degraded coherence.

The good coherence (gamma^2 = 1.0) across the range of 0.07 Hz to 20 Hz shows the region where the two instruments produced nearly identical outputs. From this, we infer a low contribution of instrument self-noise in this range.

In the frequency ranges where the coherence drops off, the instrument self noise is larger. The shape of the coherence plot is partly an artifact of the dataset I chose. During this time there was very little energy measured in the lowest frequency range. When re-running this script against data with several large distant earthquakes, the coherence was much better across all frequencies.

Yuma-2 coherence plot

It's also interesting to note the phase difference between the two units. I suspect some of the phase shift from 1-20 Hz could be due to the differences in the coils. In addition to their different force constants, Unit 2 has a significantly higher inductance. In my Spice simulations, the coil leakage inductance had an notable effect on phase margin of the loop.

Yuma-2 coherence phase plot


Other seismomenter builders are doing exciting things with their instruments. Gary Oliaro has some fascinating pages about his work using Yuma to measure solid-earth tidal effects. See the moon pulling on Princeton, New Jersey. Also, check out his detection of earth normal modes using two Yumas operating coherently. 

Larry Cochrane has a nice live page that automatically updates, showing earthquakes from around the world captured using his equipment.

Other local builders have their live Yuma seismometer data online, including Peter Rowe in Los Altos, and Alan George in San Jose.

And, of course, Brett Nordgren has done a huge amount of work and provided many detailed reports on the theory of operation, electro-mechanical simulation, calibration, and optimization of this family of instruments. His extensive archive contains a wealth of information.  For me personally, it was these documents that initially caught my attention, piqued my interest, and convinced me that I wanted to build a FBV seismometer. A special thanks to him for being so helpful and supportive, and providing me with critical materials for construction.


I welcome your comments or questions.   Email me at brian@groundmotion.org

Last updated: 11/20/2017