Hello,
Thanks for the pointers with the PDF file.=20
Thanks for the tip - I've been playing around with a Texas Instruments =
TSL230 chip - http://www.taosinc.com/pdf/tsl230.pdf which is a light to =
frequency converter - which if you have enough time between samples may =
possibly be used as a photon counter???. One of the problems in using =
an inferometer outside of the resolution issue is that the arc of the =
boom would tend to throw the alignment required out of line. =20
I saw really neat web page @ =
http://www.users.globalnet.co.uk/~blootl/trackers/sunflower.htm - some =
folk in the U.K. have been constructing very large parabolic mirror to =
point at the sun, > 40 KW outputs... The TSL230 would make for a =
dandy solar alignment sensor.
Here on the tundra of Minnesota, I've just built my second 24 bit ADC =
board - sent it off to my brother in Canada for eval. I'm using a 30K =
turn coil and a (1,10,100,1000 x ) programmable gain amp - and a stamp =
to control it all - sending 10 hz data to my PC with a VB front end that =
displays my traces in realtime.... I get quite a signal just rotating =
the assemby away from any magnet - just using the earth magnetic feild =
to interact with the coil... The whole thing sits on a 2 x 3 inch board =
running of a single sided supply. I steal a +12 v line from the PC to =
run it.
Jim
----- Original Message -----=20
From: ChrisAtUpw@..........
To: psn-l@.................
Sent: Saturday, November 17, 2001 6:48 PM
Subject: Re: Publication on the Web
In a message dated 17/11/2001, jimesler@.......... writes:=20
Does anyone have any experiences in building an inferometer for =
measuring=20
displacement in seismographs?=20
Jim Esler
Dear Jim Esler,=20
The problem with using methods which depend on the wavelength of =
light is that you are ultimately limited by this dimension, which is =
about 0.6 micron. When observing seismic signals, you will probably want =
a resolution of better than 1/20 of this. While optical sensors which =
measure to small fractions of a wavelength can be bought, they are =
neither simple nor cheap.=20
The wavelength limitation may be largely avoided by using a =
fairly intense and constant light source to illuminate a pair of =
silicon photodiodes through a moving shutter attached to the seismometer =
arm. The difference in the photocurrents is measured, filtered and =
amplified. This 'photon counting' method is also simpler in principle =
than interferometer techniques. Hope that this helps.=20
Regards,=20
Chris Chapman =20
Hello,
Thanks for the pointers with the PDF file. =
Thanks for the tip - I've been playing around with a =
Texas=20
Instruments TSL230 chip - http://www.taosinc.com/pdf=
/tsl230.pdf =20
which is a light to frequency converter - which if you have enough time =
between=20
samples may possibly be used as a photon counter???. One of the =
problems=20
in using an inferometer outside of the resolution issue is that the arc =
of the=20
boom would tend to throw the alignment required out of line. =
I saw really neat web page @ =
http://www.users.globalnet.co.uk/~blootl/trackers/sunflower.htm =
-=20
some folk in the U.K. have been constructing very large parabolic mirror =
to=20
point at the sun, > 40 KW outputs... The TSL230 would =
make for a=20
dandy solar alignment sensor.
Here on the tundra of Minnesota, I've just built my =
second 24=20
bit ADC board - sent it off to my brother in Canada for eval. I'm =
using a=20
30K turn coil and a (1,10,100,1000 x ) programmable gain amp - and a =
stamp to=20
control it all - sending 10 hz data to my PC with a VB front end that =
displays=20
my traces in realtime.... I get quite a signal just rotating the =
assemby=20
away from any magnet - just using the earth magnetic feild to interact =
with the=20
coil... The whole thing sits on a 2 x 3 inch board running of a =
single=20
sided supply. I steal a +12 v line from the PC to run =
it.
Jim
----- Original Message -----
From:=20
ChrisAtUpw@.......
Sent: Saturday, November 17, =
2001 6:48=20
PM
Subject: Re: Publication on the =
Web
In a =
message dated=20
17/11/2001, jimesler@..........=20
writes:
Does anyone have any experiences in building an =
inferometer for=20
measuring
displacement in seismographs?
Jim =
Esler
Dear Jim Esler,=20
The problem with using =
methods=20
which depend on the wavelength of light is that you are ultimately =
limited by=20
this dimension, which is about 0.6 micron. When observing seismic =
signals, you=20
will probably want a resolution of better than 1/20 of this. While =
optical=20
sensors which measure to small fractions of a wavelength can be =
bought, they=20
are neither simple nor cheap. =
The=20
wavelength limitation may be largely avoided by using a fairly intense =
and=20
constant light source to illuminate a pair of silicon =
photodiodes=20
through a moving shutter attached to the seismometer arm. The =
difference in=20
the photocurrents is measured, filtered and amplified. This 'photon =
counting'=20
method is also simpler in principle than interferometer techniques. =
Hope that=20
this helps.
Regards,=20
Chris Chapman=20
=
=
=20
Larry Cochrane <cochrane@..............>