PSN-L Email List Message
Subject: Re: New subscriber
From: ChrisAtUpw@.......
Date: Sun, 27 Feb 2005 22:52:33 EST
In a message dated 27/02/2005, jpopelish@........ writes:
I am an electrical engineer residing in the Shenandoah valley in central
Virginia. Analog circuit design is my forte. I have been interested in
geology, volcanism and earthquakes for a long time. After discussing seismometer
amplifiers with someone, recently, in sci.electronics.design, I started
searching the web for home built seismometer and sensor designs.
One thing that struck me about many of the sensor designs is their lack of
optimisation and sophistication. Either this means that the sensor is not the
limiting part of most designs or else it means that considerable improvement
is possible.
Hi John,
Welcome! I can't comment on your discussions - I can't find the website
you quote. Seismometer amplifiers do need quite specialised design with low
noise, low drift, high gain and good filters with a low pulse overshoot.
I don't know where you are finding the 'many' amplifier designs? There
is one on Larry's website which uses LT1007s and is optimised. You need to
optimise both current and voltage noise sources. LT1007s, OP07s and OP27s can
all give satisfactory performance. If you wish to use very long periods where
1/f noise is a limitation, MAX432 and chopper amp circuits are available.
Don't confuse apparently simple with unsophisticated! You are trying to get the
amplifier noise a factor of 10 lower than the seismic noise. The ready
availability of inexpensive but powerful NdFeB magnets has allowed the use of
smaller sensor coils and magnets with increased sensitivity.
After puzzling a bit over how I might design an inductive sensor that would
improve upon the simple solenoidal coil and horse shoe magnet approach, I
think I have come up with a more sensitive design that also has noise cancelling
capability that will help it reject line generated fields (AC hum),
variations in the Earth's magnetic field caused by the solar wind and lightning
magnetic fields. This is based on making two similar coils that produce equal and
opposite signals when exposed to large, common, external fields, but produce
equal and aiding signals when exposed to the relative movement between the
coils and magnet structure. The magnet structure also has no net external
field to interact with the geo field that might interact with the seismometer
boom.
I have purchased a batch of NeFeB magnets on EBAY and am awaiting a quote
for construction of the 6 iron pole pieces to make one of these fist sized
sensors. I will make the coil forms and wind the coils, myself. I will also
make the signal amplifier and filter. If that all comes together, I will take a
shot at building a Lehman type
horizontal, long period pendulum.
I suggest that you consider 1" square NdFeB magnets in a quad formation,
NS opposing SN, in between two 1/4" thick rectangular mild steel plates, say
3.5" long by 2" wide. You wind a flat rectangular coil to half cover the
magnet poles, say ~1" square. The coil is completely screened by the soft iron
backing plates, which should be earthed to the same point as the seismometer
frame and the amplifier inputs. You can use the same layout, but with thicker
rectangular 1" x 1/2" magnets for an Al or Cu inductive damping plate. This
design gives very low stray external magnetic fields. Try it - you will like
it!
AC hum is fairly low and is strongly filtered by your 3 to 10 Hz
amplifier filters. You should use woven screen connecting cable. The main problem in
domestic situations is in limiting interference coming in through the
utility supply and from various domestic sources. Fridges, cookers and electrical
heating systems can produce large surges. You may benefit from a line filter.
It is preferable to make the seismometer arm and weight using non magnetic
materials. Stainless steel water pipe is quite useful for the arm and you can
buy brass screw clamp fittings quite easily, to fit.
Don't use a knife blade or a point suspension. Ball on a flat, crossed
cylinder, crossed wire and crossed foil suspensions are all OK. Single wire
and single foil (Cardan hinge) may also be OK. See
_http://pages.prodigy.net/fxc/_ (http://pages.prodigy.net/fxc/) _http://pages.prodigy.net/fxc/JC.html_
(http://pages.prodigy.net/fxc/JC.html)
_http://www.jclahr.com/science/psn/gldn_psn.html_ (http://www.jclahr.com/science/psn/gldn_psn.html) &
_http://physics.mercer.edu/petepag/MKXVII.pdf_
(http://physics.mercer.edu/petepag/MKXVII.pdf)
I also have a DATAQ DI-194-RS to hook it up to a computer but no software
other than what came with that unit.
You won't be very happy with a 194 for very long, but it is a start. You
do really need 16 bits resolution for this type of work. Remember that you
also need good triggering, recording, display and data analysis software. And
you do need 0.1 sec timing accuracy. Calculate how much storage space you
would need at 20 sps for a single day?
Eventually I want to add an optical beam sensor that will make the unit act
as a tilt meter (true DC operation, similar to the differential capacitive
bridge type pickup, but with much simpler support circuits) and allow
experiments with feedback using the
original inductive sensor as a linear motor. This should keep me busy for a
year or more.
You might find some information to interest you at
_http://jclahr.com/science/psn/index.html_ (http://jclahr.com/science/psn/index.html) You can
make OK optical sensors using large area photodiode pairs (7sq mm) and a
tungsten filament lamp with either a resistance or a voltage stabilisation circuit.
Infra red LEDS change their output by about a factor of 5 at constant current
between 0 and 100 C, so you would need to use additional photodiode
stabilisation if you used one of them. I can get down to about +/- 15 nano metres of
noise, or less if I reduce the bandwidth below 10 Hz.
You can also use NdFeB magnet quads and an A3515 Hall Effect sensor. See
_http://www.geocities.com/meredithlamb/page003.html_
(http://www.geocities.com/meredithlamb/page003.html) Two pairs of rectangular magnets, one SN and
the other NS, are mounted on parallel soft iron backing plates connected by
mild steel bolts. The sensor is suspended in the central field join.
There are also differential capacitor designs available - if you need
sub nanometre resolution. These are a subject in themselves.
Anyway, here is some "food for thought".
Can I suggest that you visit
_http://psn.quake.net/maillist.html#archives_ (http://psn.quake.net/maillist.html#archives) and download the last few
years' letters? There is a great deal of good information and experience
detailed therein.
Regards,
Chris Chapman
In a message dated 27/02/2005, jpopelish@........ writes:
<=
FONT=20
style=3D"BACKGROUND-COLOR: transparent" face=3DArial color=3D#000000 size=
=3D2>I am an=20
electrical engineer residing in the Shenandoah valley in central=20
Virginia. Analog circuit design is my forte. I have been intere=
sted=20
in geology, volcanism and earthquakes for a long time. After discuss=
ing=20
seismometer amplifiers with someone, recently, in sci.electronics.design,=20=
I=20
started searching the web for home built seismometer and sensor designs.&n=
bsp;=20
One thing that struck me about many of the sensor designs is their=
=20
lack of optimisation and sophistication. Either this means that the=20
sensor is not the limiting part of most designs or else it means that=20
considerable improvement is possible.
Hi John,
Welcome! I can't comment on your discussions -=20=
I=20
can't find the website you quote. Seismometer amplifiers do need quite=20
specialised design with low noise, low drift, high gain and good filters wit=
h a=20
low pulse overshoot.
I don't know where you are finding the 'many'=20
amplifier designs? There is one on Larry's website which uses LT1007s and is=
=20
optimised. You need to optimise both current and voltage noise sources. LT10=
07s,=20
OP07s and OP27s can all give satisfactory performance. If you wish to u=
se=20
very long periods where 1/f noise is a limitation, MAX432 and chopper amp=20
circuits are available. Don't confuse apparently simple with unsophisticated=
!=20
You are trying to get the amplifier noise a factor of 10 lower than the seis=
mic=20
noise. The ready availability of inexpensive but powerful NdFeB magnets=
has=20
allowed the use of smaller sensor coils and magnets with increased=20
sensitivity.
<=
FONT=20
style=3D"BACKGROUND-COLOR: transparent" face=3DArial color=3D#000000 size=
=3D2>After=20
puzzling a bit over how I might design an inductive sensor that would impr=
ove=20
upon the simple solenoidal coil and horse shoe magnet approach, I think I=20=
have=20
come up with a more sensitive design that also has noise cancelling capabi=
lity=20
that will help it reject line generated fields (AC hum), variations in the=
=20
Earth's magnetic field caused by the solar wind and lightning magnetic fie=
lds.=20
This is based on making two similar coils that produce equal and opposite=20
signals when exposed to large, common, external fields, but produce equal=20=
and=20
aiding signals when exposed to the relative movement between the coils and=
=20
magnet structure. The magnet structure also has no net external fiel=
d to=20
interact with the geo field that might interact with the seismometer=20
boom.
I have purchased a batch of NeFeB magnets on EBAY and am awai=
ting=20
a quote for construction of the 6 iron pole pieces to make one of these fi=
st=20
sized sensors. I will make the coil forms and wind the coils,=20
myself. I will also make the signal amplifier and filter. If t=
hat=20
all comes together, I will take a shot at building a Lehman=20
type
horizontal, long period pendulum.
I suggest that you consider 1" square NdFe=
B=20
magnets in a quad formation, NS opposing SN, in between two 1/4" thick=20
rectangular mild steel plates, say 3.5" long by 2" wide. You wind a flat=20
rectangular coil to half cover the magnet poles, say ~1" square. The coil is=
=20
completely screened by the soft iron backing plates, which should be earthed=
to=20
the same point as the seismometer frame and the amplifier inputs. You can us=
e=20
the same layout, but with thicker rectangular 1" x 1/2" magnets for an=20=
Al=20
or Cu inductive damping plate. This design gives very low stray external=20
magnetic fields. Try it - you will like it!
AC hum is fairly low and is strongly filtered b=
y=20
your 3 to 10 Hz amplifier filters. You should use woven screen=20
connecting cable. The main problem in domestic situations is in limiting=20
interference coming in through the utility supply and from various domestic=20
sources. Fridges, cookers and electrical heating systems can produ=
ce=20
large surges. You may benefit from a line filter. It is preferable to make t=
he=20
seismometer arm and weight using non magnetic materials. Stainless steel wat=
er=20
pipe is quite useful for the arm and you can buy brass screw clamp fittings=20
quite easily, to fit.
<=
FONT=20
style=3D"BACKGROUND-COLOR: transparent" face=3DArial color=3D#000000 size=
=3D2>I also=20
have a DATAQ DI-194-RS to hook it up to a computer but no software other t=
han=20
what came with that unit.
You won't be very happy with a 194 for very lon=
g,=20
but it is a start. You do really need 16 bits resolution for this type of wo=
rk.=20
Remember that you also need good triggering, recording, display and data=20
analysis software. And you do need 0.1 sec timing accuracy. Calculate how mu=
ch=20
storage space you would need at 20 sps for a single day?
<=
FONT=20
style=3D"BACKGROUND-COLOR: transparent" face=3DArial color=3D#000000=20
size=3D2>Eventually I want to add an optical beam sensor that will make th=
e unit=20
act as a tilt meter (true DC operation, similar to the differential capaci=
tive=20
bridge type pickup, but with much simpler support circuits) and allow=20
experiments with feedback using the
original inductive sensor as a line=
ar=20
motor. This should keep me busy for a year or more.
You might find some information to interest you=
at=20
http://jclahr.com/science/=
psn/index.html You=20
can make OK optical sensors using large area photodiode pairs (7sq mm) and a=
=20
tungsten filament lamp with either a resistance or a voltage stabilisat=
ion=20
circuit. Infra red LEDS change their output by about a factor of 5 at consta=
nt=20
current between 0 and 100 C, so you would need to use additional photod=
iode=20
stabilisation if you used one of them. I can get down to about +/- 15 nano=20
metres of noise, or less if I reduce the bandwidth below 10 Hz.
You can also use NdFeB magnet quads and an A351=
5=20
Hall Effect sensor. See
http://www.geoci=
ties.com/meredithlamb/page003.html Two=20
pairs of rectangular magnets, one SN and the other NS, are mounted on=20
parallel soft iron backing plates connected by mild steel bolts. The sensor=20=
is=20
suspended in the central field join.
There are also differential capacitor designs=20
available - if you need sub nanometre resolution. These are a subject in=20
themselves.
Anyway, here is some "food for thought".
Regards,
Chris Chapman
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