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|    sci.optics    |    Discussion relating to the science of op    |    12,750 messages    |
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|    Message 11,541 of 12,750    |
|    Phil Hobbs to haiticare2011@gmail.com    |
|    Re: Simple lock-in design for Oz-type me    |
|    13 Jan 14 12:31:22    |
      From: pcdhSpamMeSenseless@electrooptical.net              On 01/12/2014 10:32 PM, haiticare2011@gmail.com wrote:       > On Sunday, January 12, 2014 8:22:18 PM UTC-5, Phil Hobbs wrote:       >> On 1/12/2014 12:51 PM, hai...@gmail.com wrote:       >>       >>> Oz: When you control both the emitter (eg led) and sensor (eg PD       >>> with       >>       >> blah blah       >>>       >>       >>> An interesting twist on this lock-in is the algorithm described       >>> by       >>       >>> Horowitz in his Art of Electronics, ca. p. 1027. The algorithm       >>> is so       >>       >>> simple it is mind-bending: Just add many measurements, and the       >>       >>> "grass" on top of the mountain will become visible. No averaging       >>       >>> involved in its execution. I know this has been used in the       >>> Hubble       >>       >>> telescope, and wonder if anyone has used this in more mundane       >>> apps.       >>       >>>       >>       >>> Horowitz explains this by noting that the noise increases as the       >>> sqrt       >>       >>> of number of observations, but the buried signal increases in a       >>       >>> linear fashion. So, if the measurement value is 100 with noise       >>       >>> fluctuation 5, and the signal is say .01, then after 10exp6       >>       >>> measurements, the signal is now 10,000 and the noise fringe       >>> 5,000.       >>       >>>       >>       >>> The signal value will be 100 million from the addition, so a       >>       >>> microprocessor seems a good way to do this.       >>       >>>       >>       >>       >>       >>       >>       >> The only difference between adding and averaging is dividing by       >> the       >>       >> number of measurements. The SNR improvement is unchanged. This       >> has       >>       >> been known since the time of Gauss, at least.       >>       >>       >>       >> Cheers       >>       >>       >>       >> Phil Hobbs              > hmmm Horowitz (page 1027 AOE) sez: "...the average value contributed       > by noise is quite irrelevant: all that matters is the fluctuations       > of the average value around the mean." He then goes on to give an       > example of Mossbauer spectroscopy which is identical mathematically       > to what I was talking about. If you notice the graph (page 1028),       > the values are just added to form a noise floor after many samples       > are taken. Now, you could just average the final accumulated number       > after 100,000 sweeps (in his example), but that would reduce the       > effective SNR here, as I see it. In any case, the magic occurs here       > in the addition process forming a low "fuzz" noise floor. To say it       > is the same as s simple average may confuse, since the "average       > averager" may just take enough samples to have his number SD settle       > down, whereas there can still be a signal buried in the pile. Just       > my reading.              So what do you think is the difference between averaging and summing?              IIRC that H&H plot is on a semilog scale, so the division just moves the       curve down a bit.              This is all just math, you don't have to wave a dead chicken over it.              Cheers              Phil Hobbs              --       Dr Philip C D Hobbs       Principal Consultant       ElectroOptical Innovations LLC       Optics, Electro-optics, Photonics, Analog Electronics              160 North State Road #203       Briarcliff Manor NY 10510              hobbs at electrooptical dot net       http://electrooptical.net              --- SoupGate-Win32 v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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