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 =20Hello,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 PMSubject: Re: Publication on the = WebIn 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@..............>