Monday, May 13, 2019
Screwed Up by Photobucket
Fortunately, I never used Photobucket (or any other site) for my primary storage of photos. I maintain my own local storage and at least two backups of all images. The online sites are mostly for convenience of being able to show others my photos and linking to pages such as this.
I got fed up with Photobucket and deleted my account and all images on their site. I had forgotten I used their site for images on this blog. Other than more recent posts all my images here are now broken links. I have all the original photos. I just need to figure out what photo went to what post. I will try to fix those over the next few months.
Just goes to show don't trust any third party storage service. Be it for photos, music, files or what ever. This is especially true if using a "free" site. I don't trust my paid sites either. They could change policy or just go out of business at any time. Always maintain your photos somewhere where you have control.
Saturday, February 09, 2019
Common Mode Choke for VLF
I use a drill to twist the wires before winding the core. Clamp one end of two wires into a vise. Clamp the other end into the drill chuck and let her wind away.
Differential mode loss is less than 1 DB. Common Mode loss was taken with my MDO3000 scope using the function generator to generate flat broadband noise from a few Hertz to past 2 MHz. This image stops at 2 MHz.
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| Common Mode Response |
Frequency KHz Loss (DB)
25 -13
50 -20
100 -27
250 -33
350 -37
450 -39
500 -40
700 -42
1000 -42
1200 -41
1500 -39
2000 -37
This will be installed in a junction box that is near the feed point of the antenna. It is about 5 feet away from the connection point. If there are any noise signals on the coax line this should reduce them.
Tuesday, February 05, 2019
630 Meter Interference
It will be interesting to find out what this is. I suspect this is a television or something in the room with a television that household turns on in the evening and turns it off when they go to bed. So far I have not heard this noise during the day (Monday - Friday).
To track this down I plan on taking a ferrite rod and build a loop stick antenna. Those have a sharp null off of the end of the rod. Walking around the neighborhood I hope to be able to use that null to at least locate the house where it is coming from. Of course I need to make sure it is not something within my own home. That would be an easy fix if that was the case. Since this shut down last night around 11:15pm I can not think of anything in the house that would have done that last night.
Ground Probe Antenna
Ground probe antenna which some call them Earth Probe Antenna. It consists of a long wire terminated with ground rods at each end. Looks similar to a Beverage antenna which is a very long wire terminated at the end. The wire being only a few feet off of the ground. These are low noise antennas directional off the end. Best used for DX on 160 meters as their directivity and pickup of local noise is much less than an Inverted-L for example.
The Ground probe antenna is used for reception of ELF and VLF signals. This post will describe the one I put out on my property in the suburbs. My back yard is around 175 feet wide and I was able to run a wire out 158 feet (41 meters). For now the wire is just laying on the ground. I drove 8 foot ground rods at each end. I connect to the antenna approximately in the middle. I am not sure how to feed this antenna so I did so in the middle as that was a convenient location. Some on suggested the impedance magnitude was around 1000 ohms. With further measurements I think it is more like 500 ohms.
I have in my junk box a ferrite core of unknown properties. I measured the AL value at 6490 mH / 1000 turns. The material appears to be "P" or "F" ferrite used in switching power supplies running under 1.5 MHz. I am feeding the antenna with RG-6 cable. I used 50 turns on the antenna and 14 turns connected to the RG-6. I am going to change that when I get a chance assuming a 500 ohm Zmag rather than 1000 ohms.
I drove the ground rods below grade with a 12" long section of 4" PVC at the top with a cap. The cap is flush with the ground so I can run the mower over the top. I can still get to the ground rod connection by removing the cap. I did the same for the coax connection in the center. The transformer sits inside of the 4" PVC.
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| Ground Rod below grade in 12" PVC pipe so I can get to the connections |
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| Cap covers rod and transformer connections |
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| Transformer for feed point to RG-6 coax |
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| 630 Meter WSPR station I heard the night of February 4, 2019 |
Sunday, January 13, 2019
Antenna Voltages Near Broadcast Stations - 160 Meters
Recently I have been improving my 160 meter antenna system. I made a few changes to the Inverted-L antenna by spacing it farther off of the tower and getting the end wire out of the tree. I still need to get the end wire higher up in the tree. The wire is around 134 feet long. 80 feet go up the tower and the remainder horizontally toward a tree to the south. The end of that wire is only about 25 feet above the ground. It should be more horizontal. That tree is much taller but I can't get up in it any higher without a bucket truck or a man-lift.
I also added eleven radials fanned out over the back yard. The radials are 67 feet long. There is a reason for that which I should document in a future post.
The 160 meter band is just above the AM broadcast band. I live with in 2 miles of the big three Dayton, Ohio AM radio stations: WING, WHIO, and WONE. These are 5000 watt stations running omni directional antenna during the day and directional at night. The inverted-L picks up a log of RF during the day when the stations are running an omni pattern. At night the directional pattern appears to be away from me as the signal level drops for all three stations.
For example, looking at WHIO (1290 KHz) using a frequency selective volt meter I see +16 DBm during the day on the inverted-L. At night it drops below 0 DBm.
Today I hooked up four 1N4148 signal diodes in a full wave bridge configuration. I hooked that to the inverted-L antenna. I get 38 volts open circuit from the diode bridge. Short circuit current is 8 ma. I placed an LED across the diode bridge output. It lights the LED right up!
Monday, July 07, 2014
Looking At My Antennas With The HP8753B
Using the HP 8753B Vector Network Analyzer I took a look at what my Classic 33 Yagi and 3-band fan dipole looks like from the shack. The Classic 33 is my original that dad got used back in the 70's It was refurbished once and installed at this QTH in 1989. The antenna has not been touched since. The feedline is Belden 9913 which was installed in 1989. Getting concerned that this air core coax may have water in it after all these years. For today's test the outside conditions are dry and have been for a couple of days. The Fan Dipole I put up last year. It consits of three dipoles feed from a common point. The dipoles are for 40, 30, and 17 meters. Dipole spacing and length of the elements are from a military document (Army I think) I found online. This document was written back in the 50's or 60's if I recall. It is installed as a sloper off of the tower favoring the west. I used the old 9913 coax that feed the 40-meter inverted V that this antenna replaced.

Looking at the Classic 33 first
I don't have a way to download the screen shot of the VNA so I used my Canon 30D camera to take a picture of the screen. I see I need to work on the focus. I used a tripod in front of the VNA but it was easily moved out of postion. If I am going to continue to use the camera I need to build a fixture that attaches to cart that holds the VNA.
The first screen shot is a Smith Chart view on 20 meters.

I was playing with the buttons on the VNA so now on to the Return Loss and SWR plots.
The SWR on the Classic 33 is not very broad on 20 meters. The yagi elements were installed favoring the voice part of the band. So the low end of the CW band suffers. SWR is 3.2:1 at 14.0 MHz, 1.16:1 at 14.2 MHz, and 1.6:1 at 14.3 MHz


15 Meters is better with the SWR ranging from 1.75:1 at 21.0 MHz to 2.0:1 at 21.450. Best SWR at 1.43:1 is at 21.160 MHz


10 meters is a wide band. The Classic 33 was intended to be used in the lower part of the band below 29 MHz. Installed for the SSB part of the band SWR ranges from 1.87:1 at 28.0, 1.17:1 at 28.3 MHz, 1.57:1 at 28.5 MHz, and 2.28:1 at 29.0 MHz. This image shows the return loss as well as the SWR in ().

The results of the tests look as I remember them when the antenna was installed at this QTH. After I made these tests I disconnected the yagi and placed a short on the end of the feedline. Using a return loss measurement and calculating the length of the coax line I came up with the following:
Length of line = 156 Feet
Loss measured at 50 MHz = 2.4 DB
9913 has a loss at 50 MHz of 0.9 DB/100 Foot according to one datasheet I found online. At 156 feet the loss per this specification is 2.8 DB. So this loss is within spec give or take my measurement error.
My notes from the installation back in 1989 indicates the disance from my connector panel in the shack to the connector at top of the tower is 136 feet. All the measurements I have made using the VNA or an MFJ analyzer show the length of my line to be 156 feet. Not sure why I have a discrepancy of 20 feet. I plan on changing out this feedline so I will measure what I pull out and see if my VNA or my notes are correct.
Now the Fan Dipole
Looking at the Fan Dipole return loss from 5 to 55 MHz you can see the three bands. Also a good return loss is noted around the 6 meter band at 49.5 MHz just a little shy of our allocation.

Looking at 40 meters the SWR ranges from 1.34:1 at 7.0 MHz to 1.8:1 at the top of the band, 7.3 MHz.

Moving to the 30 meter band. SWR is highest at the lower end of the band. 1.46:1 at 10.1 dropping to 1.20:1 at 10.180

On 17 meters the lowest SWR of 1.03:1 is below the band at 17.740 MHz. For the lower band edge of 18.068 the SWR is 1.7:1 rising to 1.8:1 at the top of the band. If I get ambitious I may try to shorten the 17 meter dipole a bit to pull the lower SWR inside of the band.

Monday, February 21, 2011
GE Mastr II Repeater
I am converting a GE Mastr II base station from commercial service to amateur radio repeater service. The original system was used as a base station up around 155 MHz. The GE is specified from 138 to 174 MHz but there were some component changes in models that operated below 150 MHz. Looking at web sites on converting these systems only the receiver has a few capacitors that need changed for optimum performance. The first step is to confirm the unit is working as it came out of service. Cleaning up the system I found there had been a mouse nest in the power supply. Had to clean that out. Apparently no damage caused by the unwelcome guests. Now on to testing the system. Testing the transmitter I found the output power was only 1.5 watts. That is a little off from the specified 100 watt output. There is a known issue where a strap that was placed between two PC boards to couple the output power from the finals to a filter develops a hairline fracture. The symptoms pointed to that as a possible problem. Turns out that was not the case. Since this was used in non-repeater service there is an antenna change over relay on the output. The relay had gone bad. Since I am using this for repeater service I don't need the relay so I pulled it off of the board and jumpered across it with a small length of RG-316 coax. Problem solved. I can develop the full 100 watt output now. For testing purposes I set the power output to 50 watts while I am doing the conversion. Next step will be check the receiver.
Friday, April 16, 2010
Catalog Filters
Minimum Fo = 494.1 MHz
Maximum Fo = 586.0 Mhz
Other specs remained about the same but the insertion loss and bandwidth was increasing as I approched the upper limit.
For this filter I can pull about 8% from center but the catalog frequency was already near the top of the range. This would be unknown to the purchaser until after they examined the product.
If you need a filter check the catalog offerings from Digikey and Mouser. You may luck out and find something that might tune to the desired frequency but I would not try to go beyond 8 to 10 percent.
For reference this part was Toko type 7HW, Part number # 252HXPK-2736F (Digikey #TK3307-ND)
Thursday, April 08, 2010
Followup on Cheap Cables
From the photograph you can see there is minimal copper braid but an inner foil around the center dielectric. Looking into the cut-a-way connector body I found the crimp was applied metal against cable jacket. There were strands of the copper braid sandwiched between the metal connector body and the cable jacket. That was the extent of the ground connection. The foil did not touch the connector body as the inner chamber of the connector widened out past the cable jacket. I suspect the shield connection had been compromised. The bad connection could have been caused a number of factors such as the copper braid being pushed into the jacket, corrosion of the copper wires, or breakage of the wires.

Moral of the story is if you obtain cheap cables they may work fine but keep in mind they may have limited life. Don't be afraid to chuck them at first sign of trouble. I still prefer my homemade cables made from LMR-240 Ultraflex and the correct connectors for that cable type.
Tuesday, March 30, 2010
Cheap Cables
Moral of the story. Buy good cables they will save you headaches in the long run.
Wednesday, September 23, 2009
ABS problems on the van
C0281 (chassis code - ABS) Brake Switch Circuit
C0223 (chassis code - ABS) Rt Front Speed Signal Erratic
I suspected the right front wheel so this confirms it. The test procedures specify resistance and voltage readings for the sensor. Getting the voltage reading is going to be a trick as I can not spin the front wheel as I have all wheel drive. I will have to disable the ABS then rig up a cable to attach to the harness so I can roll the van down the driveway to measure the AC pulse train. The voltage is very low (approx 100 millivolts) so noise is going to be a problem even using the oscilloscope. The service bulletin indicates the signal should be at least 350 mV but this document says greater than 100 mV. So much for consistent documentation.
The procedure also measures the cable from the sensor to the electronic brake control module (ECBM). It states that faulty wire connections is a leading cause. The darn EBCM is attached to the frame under the van. That is the dirtiest place you could put the thing.
I am a little confused by the C0281 code for the brake switch circuit. The description indicates that this code may set if the there is an ABS fault of at least 500 milliseconds. That would have set by the C0223 code but then in the next line it says the code only sets if there is an open or short in the brake switch circuit wiring. For now I will assume it is setting because of the sensor signal. Fix that and then see if C0281 comes back.
The last item in the correction chart is to replace the ECBM. Unfortunately you have to have a scan tool that communicates to the device. Consumer scan tools only read diagnostic codes. You need on of the expensive units to talk to the devices. You have to set the tire diameter for the vehicle in the ECBM. Crap! If that is bad it is back to the dealer to replace that darn thing. I bet they get a lot of $$$ for that module.
Over the weekend I hope to get a chance to investigate the sensor/wiring.
Sunday, September 20, 2009
UPS Batteries
Saturday, September 19, 2009
UPS Failure!
I test the batteries using a computerized test fixture. This is a device by West Mountain Radio. Plugs into the USB port on the PC and by running the provided software you can do a load test and see if the battery meets specification. You can see the resulting chart after the test on the first battery. You set the load current as indicated by the specification. Most batteries of this type are tested over a 10 or 20 hour rate. Power Sonic lists the spec for both 10 and 20 hours so I used the 10 hour rate. For a 7.2 AH battery that is 0.700 Amps. They also specify the "dead" voltage which is typically 10.5 volts for a 12 volt battery at this load current. As you can see from the chart I got 8 Ah out of the battery by the time it hit 10.5 volts. So battery 1 is good. This battery goes on the charger and I connect up the second. At ten hours a test this will take a little time.

Chart after test of first battery

Batteries ready for testing. Battery #1 connected to the test fixture

Batteries as wired up in the UPS unit
New Toy
I have completed the functional tests out of the manual. The unit appears to be in good shape and calibration.

Wednesday, September 02, 2009
The SUN's solar activity and climate change
This is comment was in a DX news letter that follows along with what I found when I took the propagation course.
Out in space the sun remains on a record pace at 51 days without sunspots, and no expectations of any change soon. We’ll be in the top 3 longest quiet periods by Wednesday evening (tied with 54 days from 1879) and by late next week we’ll head into the 2nd position as we surpass 63 days from 1901. The daily solar observations began in 1849, but we know from other observations between 1400 and 1830 that these
periods of sunspot minimums were associated with a 400-year stretch known as the Little Ice Age. The only problem with observations from that time is that there were no telescopes and satellites with the observational power we have today. In other words, the long periods without sunspots are even more impressive now because we can pick out the smallest sunspot, ones that would have been missed 100 to 200 years ago. We
won’t know if this is true for a long time, but at this point there is no reason to discount the idea that we’re heading into another Little Ice Age, or possible a major ice age. Time will tell…
Sunday, April 29, 2007
Testing ERA-5 MMIC for use as a multiplier
ERA-5 gain below 1GHZ = 20 DB
1 DB compression = +17.5 DBm
Input 738 MHz into MMIC at +6 DBm and +2 DBm drives the amp well into compression. No attempt was made to optimize the output for a particular harmonic or to suppress the fundamental. The output capacitor was 12 pf to favor the upper frequencies. Results varied depending on the input frequency. The data below is for 738 MHz. At 571 MHz the 5th harmonic with +2 DBm input was -20 but had a lot of “grass” around the carrier. Lowering the input to +1 DBm dropped the harmonic to -30 DBm and cleaned up the noise (or it dropped below the noise floor of the spectrum analyzer).
It appears the input should not exceed 5 DB above the 1 DB compression level or excessive noise will result.
+6 DBm input is 8.5 DB above the 1DB compression point
+2 DBm input is 4.5 DB above the 1DB compression point
Output 1 is with a +6 DBm input
Output 2 is with a +2 DBm input
Frequency(MHz) or Harmonic/Output1/Output2
738/+20/+18
X2/-2/-6
X3/+3/-12
X4/-4/-30
X5/-20/-30
X6/-42/-34
X7/-38/-46
X8/-30/-42
X9/-40/-50
X10/(below noise)/(below noise)
Tuesday, April 24, 2007
Oscillators
Other changes I made:
1. Removed the tuned transformer between the oscillator and buffer. Replaced it with a short to the DC line.
2. I moved the input capacitor of the buffer that was on the transformer link to the top of the oscillator emitter resistor.
3. I also reduced the buffer emitter resistor from 220 to 100 ohms. This helped reduce the harmonics a little. I think the buffer was also being overdriven.
I experimented with the tapped capacitors in the oscillator tank circuit. Increased them to 82 and 33 from 68 and 22 pf. No real difference. The oscillator may be slightly more stable, from a start up perspective, with the original caps so I put them back to the way they were.
In the end the 2nd harmonic is 10 db down and the others are 30 db down or more. The 5th harmonic is the last one I see on the spectrum analyzer. The input tuning on the multiplier may make these spurs a moot point. If not I will have to add an extra low pass filter after the oscillator. The final oscillator is much simpler design.
I will incorporate the design changes into the 114.2 MHz oscillator and test it out tomorrow night.
I guess I will have to go back and update the design document on my web page. That will have to wait until after Hamvention. I need to get this project done by Hamvention.









