gregory hodowanec cosmology note (1!2!94) remarks on the ia-type of gw detector circuit # 10,000-b

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  • 8/8/2019 Gregory Hodowanec Cosmology Note (1!2!94) Remarks on the IA-Type of GW Detector Circuit # 10,000-B

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    12/19/09 6:27 PMGregory Hodowanec: Cosmology Note (1-2-94) Remarks on the IA-type of GW Detector Circuit # 10,000-B

    Page 1 of 2http://www.rexresearch.com/hodorhys/94-1-2/94-1-2.htm

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    Gregory HODOWANEC

    Rhysmonic Cosmology

    Remarks on the IA-type of GW Detector, Circuit #10,000-B

    (1-2-1994)

    I. Remarks on the IA-type of GW Detector, Circuit #10,000-B

    A. Preliminary tests of the instrumentation amplifier type (IA) GW detectorcircuit #10,000-B indicated that the signals "heard" on this unit are very much

    alike those heard on Geiger Counters! This seems to imply that perhapsradioactivity effects might be "set off" by these GW signals?

    B. Some speculative thoughts on this:

    1. Possibly the GW signals present at each zenith-nadir line on earth generate the"impulses" needed to "excite" the radioactivity events?

    2. The type of signals being "heard" on the IA-type detector at this locationshould also be available at every other individual zenith-nadir line on earth!

    3. Each individual "impulse" is a rhysmonic vector force and thus should easilybe physically located well within the realm of an atomic nucleus.

    4. The energy of such rhysmonic impulses could thus be possibly transferred tocertain atomic nuclei which are momentarily unstable to enable the observedradioactivity. This should be possible since we know that GW signals also reactwith matter (mainly nuclei) to cause the observed gravity acceleration and thereaction in these capacitive detection elements. The actual process needed for theradioactivity, however, requires further study.

    II. Conclusions

    This appears to be a viable area for further study investigation and it could turnout to be of great importance. It would be nice of a few of you could try theexperiment and see if you could confirm my observations here. When timepermits I will try some other devices and continue some studies here also.

    Figure (1): Simple Differential-Amplifier Type GW Detector

    Prototype Circuit # 10,000-B (Tested 10-28-1993)

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  • 8/8/2019 Gregory Hodowanec Cosmology Note (1!2!94) Remarks on the IA-Type of GW Detector Circuit # 10,000-B

    2/2

    12/19/09 6:27 PMGregory Hodowanec: Cosmology Note (1-2-94) Remarks on the IA-type of GW Detector Circuit # 10,000-B

    Page 2 of 2http://www.rexresearch.com/hodorhys/94-1-2/94-1-2.htm

    Note 1: Input device must be current generator. Will coils work here? Evaluated with capacitorsover range of 0.1 uF to 3000 uF works okay here.

    Note 2: LP filter is now raised to a cutoff of about 100 Hz.

    Remarks:

    (1) Circuit #10,000-B is constructed within an aluminum box but the detector "device" input isbrought out in pin jacks -- to facilitate test of other devices.

    (2) Used matched 10k resistor in the buffer stage (best CMMR).

    (3) Circuit swings +/1 around 0 volts; set control was added to enable use with positive input

    chart recorders.

    (4) Circuit is basic instrumentation amplifier.

    (5) Circuit is very sensitive (large outputs).

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