| Seismometer
data
sample (archived) |
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Observations:
1. 6/10/09 The main artifact is a response proportional to
house
temperature (transient when the A/C kicks on). Ideally a
differential detector would reject this common-mode signal, but there
is enough signal gain that the artifact is visible. Prime suspect is
the temp dependence of radiant output of the IR emitter. Biased at
constant forward current, the LED output decreases at about 0.5% / deg
C.
Solution is to design compensation into the LED current source.
2. 6/17/09 Adding a positive temp. coeff has reduced the
temperature
related artifact. The main issue now is to get a proper material for
the torsion balance wire. Nylon line would not hold the penny in a
horizontal position without epoxy, which I want to avoid. Solder is
easier to work with, so I'm inclined to work with wire instead. I'll be
trying some 6-mil dia. (about 34-ga)
tungsten steel wire soon. This wire (in a thinner gauge) was used in
some balances built in the 1920's, so I'm anxious to try it out. Bonus
is that it has a low thermal coefficient of expansion.
3. 6/24/09 The thin tungsten wire has increased the
sensitivity of the torsion balance, and gives a good horizontal hold of
the penny. Resonant frequency remains a bit high - about 2 Hz. It can
be lowered by increasing the offset at which the penny is supported,
and by making the support wire thinner. When I take both measures, the
resonant freq should approach 1 Hz.
Also, tonight relocated the instrument to a more isolated area. The
DAQ device
is now connected by USB-over-IP using a Belkin F5L009 network USB hub
and a wireless bridge. The data should now have less non-seismic
interference.
4. 6/29/09 First detection of a natural seismic event, a
mild M4.3 earthquake in Baja California, 372 km away. Plot shown below.
Its peak intensity was about 18% of full scale for the instrument.
5. 7/03/09 The seismometer doesn't have a dedicated
server. As a result, I see occasional dropouts in the data due to
contention on the USB bus when I use a USB HDTV tuner to record or
watch ATSC programs off-air. The RF link is robust, but the wireless
USB driver loses the contest when hard-wired USB demands bandwidth.
6. 8/16/09 Reduced the tungsten wire diameter from six
to five mils (.005 inch). This lowered the natural resonance freq from
2.4 to
1.8 Hz.
7. 10/04/09 Raised the gain of the ADC preamp by 18 dB. This
provides enough gain that the sensitivity is no longer quantization
noise limited. Also stuffed openings at four edges of the enclosure
with foam for thermal isolation. An area that could use
further work is the geometry that the penny and flag (light block)
present to the photodetector. This can be hard to adjust, and the
resting angle of the penny/flag seems to have an impact on sensitivity.
8. 10/24/09 Made a dramatic reduction in 1/f noise by
replacing U1 and U3 with OP284 low-noise bipolar op-amps. The unit
price for these is almost $9, but the payoff is about 40dB lower noise
floor between .01-.1 Hz, and 20dB less integrated noise from 0.1-10 Hz.
There is now an output offset of 120mV due to input bias current at U3A
(see schematic);
this
will
be
addressed
at
a
later date.
9. 11/14/09 Replaced the copper penny in the pendulum with a
40 gram copper block 1 in. sq. * 1/4 in. thick. The noise floor now
shows more amplitude below 1 Hz.
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The completed seismometer board. To the right you can see the
IR emitter, magnet assembly and differential photodetector. From right
to left, in order: 1) Photodiode transimpedance amplifier/filter (dc-coupled, abbreviated "TZA" in the dataplots) 2) Instrumentation amplifier and HPF 3) Sallen-Key LPF 4) SE-to-balanced output buffer to DAQ board. The response characteristic is bandpass, with the highpass corner at 0.008 Hz and lowpass corner at 3 Hz. |
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Seismometer glamor photo, in its enclosure. It's ready to be
connected to the data acquisition board. |
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FFT of the
seismometer noise floor. The broad resonance at
2.4 Hz
is that of the damped torsion balance. The null at 4.17 Hz is the
result of a 3-point moving-average filter applied to the data, which is
sampled at 12.5 Hz. |
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The instrument's first
detection of a natural seismic event - a magnitude 4.3 quake 50 mi
south of Mexicali, Baja Calif: about 370km from my site. Here you can
see the onset of the subsurface P-waves first, followed by the much
stronger S (shear) waves at 14:41:30 PDT. The event took 60 seconds
to propagate 370 km. |
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The USGS travel
times to my site pretty much nail what was recorded above - within
a few
seconds. |
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A larger quake, M6.0 in the
Gulf of California 07/03/09, 1100 UTC, distance 902km. It is
interesting that this was
detected at all. The seismometer is oriented for E-W quakes, but this
one was at bearing 165, due south from Tempe. It would have registered
4X stronger if it had been due west. The shear wave component of this quake is lower in frequency and longer in duration than the smaller Baja quake. |
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Seismic wave travel times for
the M6.0 quake, 7/3/09. Nomenclature for the phases of seismic waves are given here. The P waves are pressure (longitudinal) waves which travel in a linear path beneath the Earth's crust. The S waves are surface transverse waves which propagate along the curvature of the Earth's crust - a longer path. |
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Four earthquakes hit the
Gulf of California on Aug 3, 2009 in succession: 5.8, 6.9, 5.0 and 6.2
Magnitude. All four can be seen in this plot. Two of these events
caused the
instrument to register a full-scale reading. There were reports that
the M6.9 was felt in Phoenix, some 900 km away. The negative and positive transients at 11:37 and 11:40 were human-caused (garage door). |
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Zoom plot of the 08/03/09
M6.9 Gulf of Calif earthquake. The longitudinal, higher frequency
pressure waves are seen first, followed by the lower frequency
transverse shear wave. This one had sustained detectable amplitude
for a half hour. |
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Detection of a M8.0
Earthquake, 09/29/09 in American Samoa - 8000 km distant. The pressure wave begins abruptly at 11:00 am (local arrival time). Other clear features are the low-frequency shear wave arrival at 11:09 am, and the Rayleigh surface wave at 11:23:30 Phoenix time. |
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Seismic wave travel times to
Phoenix for
the M8.0 quake in American Samoa, 9/29/09. |
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Detection of a M7.0
Earthquake, 01/12/10 in Haiti - a path distance of 4400 km. Unlike the M 8.0 Samoa quake above, where three distinct seismic wave components were visible, only the Rayleigh surface wave at 15:14 Phoenix time came up above the instrument noise floor. I wonder if undersea propagation enhances the LR component. |
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USGS seismic wave travel
times to
Phoenix for
the M7.0 quake in Haiti, 1/12/10. Only the "LR" component rose above
the seismometer noise floor. |
Notes:
1. Another example of a torsion balance seismometer may be found here .
2. A torsion pendulum is a special case of a compound
pendulum. The two main handles on the resonant frequency are the
moment of inertia of the weight, and the torsion constant of the wire
(inversely proportional to the wire cross-sectional area).
3. A schematic diagram for this design is here.
The
seismometer
is
completely
powered
off
of the 5V USB bus from the Labjack
U12 12-bit data acquisition
board. Supply current consumption is under 100 mA. Note: U3A should be
an AD822 and not an MC33202, since low offset is needed in the feedback
path.