Works in Progress

Here are some notes and random photos of current projects.

Entries are in reverse-time order with the newest at the top of the page.
(refresh the page for newer stuff)

I've built a prototype Infrasound detector that drives a simple bar graph. It detects frequencies below about 15 Hz. The top schematic is a low-pass filter with just a little gain. It could be modified to boost the low-frequency end for microphones that roll off below 20 Hz. AC1 is the microphone but the mic's bias resistor isn't shown. (See the Infrasound page for other preamp circuits and how to add that resistor for the mic. power.)

 

Ignore the 9 volt supply; the final circuit uses a quad op-amp running on 5 volts. The output above is represented by "V2" below.

Below is a simple precision rectifier that uses only one diode and op-amp, thanks to the nice behavior of the TLC27L7 op-amp when pegged to the bottom rail (the second op-amp is just a buffer). The red trace is the tiny 10 mV test signal (multiplied by 10 on the plot) and the violet trace is the op-amp output gracefully swinging from near-zero out to the voltage required to turn on the diode and charge the .22uF capacitor. The green trace is the voltage on the output and is right at 1 volt. The feedback resistors are selected to give this stage a gain of 100 (peak to DC) so the 10 mV peak sine wave comes out at 10 mV x 100 = 1 VDC. It's a nicely-behaved rectifier for slow AC.

 

My bar graph is a commercial display but it's quite simple inside, just two LM3914s driving 20 LEDs with a circuit right out of the National data book. But an analog meter might be even nicer. The bar graph does indicate the presence of "extra" infrasound but it's hard to beat Spectrum Lab for actually seeing what's going on. The idea here is to detect thunder for hundreds of miles. It's easy to see thunder on the spectrum so time will tell if the bar graph is equally informative.

There's little to no wind right now and there's a storm about 400 miles away. Here's what the display looks like. I think that's distant thunder, looking at Spectrum Lab, but there is nearby construction, too. Later - The wind has now picked up (the next day) and wind produces full-scale readings on the bar graph and Spectrum Lab is "lit up" below 10 Hz. These simple infrasound experiments are for calm days! Think of it as an extra "sense" that sometimes means wind and other times it means distant sound sources. When the spectrum lights up with a fairly uniform signal below 15 Hz it's probably a distant storm. Bright lines extending up the frequency scale are usually a close storm or wind, and anything with a pattern of harmonics is probably construction equipment or other man-made source.


I've calculated a new temperature conversion chart for Fenwal 10k, Curve 16 precision thermistors with a Fahrenheit conversion and 0.1C steps. Also see Fenwal 10k thermistors


Power Supply Tester

This tester is designed to test various power adapters all the way up to high-power laptop supplies. The heat sink and power transistor are simply overkill! (But it looks great!) The photo on the left shows a 9 volt supply supplying 200 mA (set by dial). The VAC is "low" meaning there's little ripple. There's a polarity-reversing adapter cable plugged in since the supply under test has a negative center pin. The power adapter on the right powers the tester. The inside view reveals the ridiculously overkill power transistor (1/2 of a dual transistor rated at 50 amps and 220 volts!) I'd recommend a more modest power darlington rated at over 5 amps and the heat sink can be much smaller since the tester only runs for a short time. Directly below the black power transistor is the display board from PicAxe.com. To the right are two protoboards from Adafruit, one with a 20X2 Picaxe and the other for the simple analog circuitry. The bottom of the case has a plastic accessory storage bottle held in place by an o-ring. A few adapters are sticking out. There are two jacks on the front for the most common connectors. The circuit is a simple current sink and an audio amplifier/detector for the ripple detection. The circuit is an adjustable current sink with a PicAXE monitoring the noise voltage and actual current.

The schematic doesn't show how the 20X2 connects to the display but that's covered in the PicAXE instructions - quite simple - just connect pin 16 from the 20X2 to the serial input on the display.  Here's the PicAXE program. You don't need to know how to program the thing; just paste this program into the PicAXE editor and click on "program."  I have a "calibrate frequency" value in mine since the display and 20X2 were having a bit of trouble communicating until I adjusted the frequency a bit. You should probably start with that line removed.


No-moving-parts field mill?


I've made modifications to the King-Sized Infrasound Microphone and the Infrasonic Converter. I've also added the output from these two projects to Live Data.


New Lightning Detectors.


 

GPS Frequency Reference


5886 Electrometer Tube Audio Amplifier

Here's a silly experiment that's an attempt to find additional uses for the 5886 electrometer tube (typically scrounged from old radiation survey meters). I wanted to see if the tubes could make reasonable front-ends for very high impedance audio amplifiers. My first attempt was a simple grounded-cathode amp and the plate linearity and bandwidth were awful leading me to believe these old tubes might only be good for "D.C." But then I tried a one-transistor feedback amplifier and the circuit came to life. Below are two versions with an added emitter-follower. They perform equally well. The top one is DC-coupled but it does rely on the plate voltage being correct for biasing the rest of the circuit. I'd go with the second circuit in most cases.

The feedback holds the plate voltage fairly constant and the resulting linearity and bandwidth are quite good. I didn't measure the distortion but a sine wave looks great whereas previously it looked like a full-wave rectified sine. The bandwidth is a surprising 400 kHz. The circuit seems to perform just about identically to the same circuit with the tube replaced by an electrometer JFET (like the 2N4117). So why not just use a 2N4117? I only have emotional answers to that question. : ) I suppose this circuit is a bit more immune to static discharge. The input impedance is "crazy high" even without bootstrapping but then it's not exactly low with the FET. If I continue I'm grasping at straws.

Note how little current the filament needs; it's not much more than a typical transistor stage.

I used a 22 megohm to ground the gate but that could just as well be a 100 gigohm or even a neon lamp with its internal radioactive isotope.


 

I moved the solar flare stuff to:  Solar Flare Project