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Disappointment with Spice and the QRP-er's favorite, the LM386

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The trusty old LM386 audio amplifier from the 70's is still used a lot in low power and portable equipment. Recently some ultra high gain circuits have been recommended that I wanted to simulate with Spice. I started with the datasheet examples for checking the quality of the model. The result was surprising.

In the data sheet one can find a minimum parts circuit, a high gain circuit, and a bass boost circuit:
Gain = 20 (26 dB), minimum parts
Gain = 200 (46 dB)
Bass Boost









There isn't any official Spice model available from the manufacturer of the chip, at least not that I have been able to find. But there is a "no-frills LM386 model" attributed to Dave Dilatush (5/30/95) so I used that and a put it in a separate LM386.sub file.

The Spice code is quite simple and listed at the end of this posting. The result is shown here in two sets of curves. The first is for the 26 dB and 46 dB amplifiers.

The first result is in the left-hand curve which shows that the high-gain version has problems with the low frequency response, so I increased the 10 μF feedback capacitor to 100 μF in the right-hand plot (between pins 1 and 8). That makes the plot almost as flat as that of the data sheet down to 100 Hz.


26 and 46 dB amplifiers according to data sheet26 and 46 dB amplifiers with 100 uF in the feedback






Second, the high frequency response is too high in the simulation compared to the data sheet shown below. The Spice model does not seem to have enough high-frequency roll-off.

Third, close inspection shows that the gain of the high-gain amplifier (the blue curve) levels off at 45.4 dB, not 46 dB. This should indicate that the open-loop gain of the Spice model is not high enough.

For comparison, the data sheet plots the responses as follows:

Finally here is the simulation of the bass boost. It is actually quite close to that of the data sheet, probably because the gain is not very high and the original plot only goes to 20 kHz.

In conclusion, in order to do simulate the LM386, there is a need for a Spice model with more roll-off at high frequencies and with a higher open loop gain.

I also observe that there is a constant current source in the LM386 model of value i1=5 mA. It must for sure be too high since the data sheet says that the quiescent current for the entire chip is min. 4 mA, max 8 mA.

Before there is any point in simulating the "Unleashing the LM386"-circuit that I introduced in Sprat (autumn 2003) or the simplified version that SM7UCZ (Johnny Apell) introduced in Sprat this spring - both based on the circuit of JF1OZL (Kazuhiro Sunamura), the Spice model needs some improvement. These circuits are also in George Dobbs, G3RJV's articles in Practical Wireless, May and July 2014.

Actually I knew that improvements are needed since I have already tried with inconsistent results. But I have the hope that some of the readers may steer me towards an improved model.





Links:

Spice code for use with TopSpice or LTSpice:
LM386 Amplifier
*
*
* LM386 Data Sheet curves simulated in TopSpice
* Sverre Holm (LA3ZA), 20 June 2014
*
**********************************
.include lm386.sub

* Step through 26, 34, 46 dB
cfeed nc4 10010uF
*rfeed nc3 100 {Rvar}; LTSPice
*.STEP param Rvar LIST 0.0110Meg; LTSpice

rfeed nc3 10010Meg; TopSPice
.STEP Rfeed LIST 010Meg; TopSpice

* Comment out for flat response (default)
*Xfeed nc3 output BassBoost

.probe
.ac dec 100101e6 ; 100 steps per decade from 10 Hz to 1 MHz
*.tran 1u3m 05u
.save vdB(speaker)
*.print ac V(speaker); LTSpice
.print ac vdB(speaker); TopSPice

vsupply vcc 0 dc 9
rsupply vcc vs 10
csupply vs 0470uF

vsignal inn 0 ac 1 sin 0.051k
rplus nc1 01e-6

* Output circuitry
csnub output snub .05uf
rsnub snub 010
ccoupling output speaker 250uf
rspeaker speaker 032

xamp inn nc1 nc2 nc3 nc4 output vs 0 lm386

cbypass nc2 00.1uf ;bypass cap for PSRR

************************************************************
* Bass boost (in LM386 Data Sheet)
.subckt BassBoost nc3 output
cfeed output 1033nF
rfeed nc3 1010k
.ends BassBoost
************************************************************
.end


Spice circuit for the LM386 (store in LM386.sub):
* NO-FRILLS LM386 MODEL
* Dave Dilatush 5/30/95
*
*http://groups.google.com/group/sci.electronics/browse_thread/thread/4acbf7a7f3c36b0f/db8514b79b5b1709
*

* lm386 subcircuit model follows:

* IC pins:23718564
*||||||||
.subckt lm386 inn inp byp g1 g8 out vs gnd

* input emitter-follower buffers:

q1 gnd inn 10011 ddpnp
r1 inn gnd 50k
q2 gnd inp 10012 ddpnp
r2 inp gnd 50k

* differential input stage, gain-setting
* resistors, and internal feedback resistor:

q3 100131001110008 ddpnp
q4 1001410012 g1 ddpnp
r3 vs byp 15k
r4 byp 1000815k
r5 10008 g8 150
r6 g8 g1 1.35k
r7 g1 out 15k

* input stage current mirror:

q5 1001310013 gnd ddnpn
q6 1001410013 gnd ddnpn

* voltage gain stage & rolloff cap:

q7 1001710014 gnd ddnpn ;
c1 100141001715pf

* current mirror source for gain stage:

i1 10002 vs dc 5m
q8 1000410002 vs ddpnp
q9 1000210002 vs ddpnp ; diode

* Sziklai-connected push-pull output stage:

q10 1001810017 out ddpnp
q11 100041000410009 ddnpn 100 ; diode D1
q12 100091000910017 ddnpn 100 ; diode D2
q13 vs 10004 out ddnpn 100
q14 out 10018 gnd ddnpn 100

* generic transistor models generated
* with MicroSim's PARTs utility, using
*default parameters except Bf:

.model ddnpn NPN(Is=10f Xti=3 Eg=1.11 Vaf=100
+ Bf=400 Ise=0 Ne=1.5 Ikf=0 Nk=.5 Xtb=1.5 Var=100
+ Br=1 Isc=0 Nc=2 Ikr=0 Rc=0 Cjc=0p Mjc=.3333 ;
+ Vjc=.75 Fc=.5 Cje=5p Mje=.3333 Vje=.75 Tr=10n ;
+ Tf=1n Itf=1 Xtf=0 Vtf=10) ;

.model ddpnp PNP(Is=10f Xti=3 Eg=1.11 Vaf=100
+ Bf=200 Ise=0 Ne=1.5 Ikf=0 Nk=.5 Xtb=1.5 Var=100
+ Br=1 Isc=0 Nc=2 Ikr=0 Rc=0 Cjc=0p Mjc=.3333 ;
+ Vjc=.75 Fc=.5 Cje=5p Mje=.3333 Vje=.75 Tr=10n ;
+ Tf=1n Itf=1 Xtf=0 Vtf=10) ;
.ends
*----------end of subcircuit model-----------

Nice radio-related stamp

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A few weeks ago I had one of my rare visits to the post office. As I was waiting, I saw a display of a new series of stamps and I just had to buy the one shown here. What caught my attention was not really the artist, but rather the Kurér portable radio.

The stamp was of course not about the radio but was issued in commemoration of the 100 year anniversary of the birth of Alf Prøysen. The English Wikipedia page has this to say about him:

Alf Prøysen (23 July 1914 - 23 November 1970), was a writer and musician from Norway. Prøysen was one of the most important Norwegian cultural personalities in the second half of the twentieth century, and he made significant contributions to literature, music, TV, and radio.

One of his main characters was "Teskjekjerringa" called Mrs. Pepperpot in English. She is shown here in the second stamp in the series. I remember this story very well from my own childhood in the 60's as told in the characteristic calm and soothing voice of Prøysen himself. The character eventually appeared in 23 different languages. The radio is of course here because this and others of his plays were very popular on radio in the 50's and 60's.

And it was this radio, the Kurér (= Courier), that made me buy the stamp. It was a highly successful portable radio from the Radionette factory in Oslo from 1950 to 1958. It has four valves and covers long wave, medium wave, ' the trawler band' and short wave. It has room for batteries (90 Volts and 1.5 Volts). But luckily it also has a built-in mains supply - the 90 Volt battery is hard to find these days. A total of 224 000 were produced and it was exported to many countries especially in the Middle East. It is very easy to repair even today.

I would think the most popular version today among collectors is the dark red one shown in the stamp. I have a grey one shown here with a simple medium wave transmitter that I have described before on top.


Read more here (Sorry, nothing but Norwegian links could be found) :

WSPR on 5 bands

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For the first time ever I have been spotted on all the five bands that my Ultimate3 QRSS/WSPR kit (G0UPL design) is transmitting on. This is after 2-3 days of transmitting.


Right now I am using the beacon for discovering if the bands should open up on 24 and 28 MHz. The other three bands, and especially the 14 MHz band, serve as references to tell me that the transmitter is working. My antenna is not so optimal so I would be surprised if I am spotted far outside Europe. It is an end-fed 5 m long half wave vertical dipole which isn't too bad for 28 and 25 MHz, and probably not very good at all on 21, 18, and 14 MHz.

New gadget measures negative resistance

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If you are like me, you appreciate electronic gadgets with dials and displays. So when I discovered this "USB detector",  I thought to myself that I really always wanted to know the voltage as well as the current consumption of my USB devices. And since it is more or less impossible to connect a multimeter, this is exactly what I need.

The device fully satisfied my curiosity. Actually one surprising result was that the charger for my Samsung Galaxy Note 8 has a negative output resistance.

With a load it outputs 5.27 Volts as shown in the top image. Usually one expects the voltage to increase when the load is removed. But for this charger the voltage dropped instead to 5.13 Volts (second image). That should mean that there is the equivalent of a series resistance of (5.13-5.27)/0.98 which is about -0.14 Ohm.

I measured other chargers also, without finding a negative output resistance, so it seems as if it applies to this particular charger only. Out of curiosity, I also measured the current consumption of my Arduino Mega to 0.08 A without any shields connects.

The unit has two outputs which are different from each other. Output 1 is a fully functional USB port, while output 2 only connects DC power. What is that good for? Well, the epanoroma blog opened my eyes to the utility of this. If you charge your phone at some public place, then this feature isolates the data port of your phone. That may protect you from being hacked.

So there you see. The €5.13 were well spent and I even learnt something new by giving in to the temptation to click "Buy It Now" on Ebay.

But why does the Samsung charger have what amounts to a negative output resistance, is it by design or by accident?

Digital Signal Processing

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The Norwegian-language "The road to the international radio amateur license" came off the press this June. It is based on the RGSB International Amateur Radio Examination Manual from 2006, which RSGB graciously allowed us to use.

But the translation has been adapted on several topics. One example is the chapter on propagation due to the need in our country for more emphasis on propagation in polar regions and in mountainous terrain. Another is a completely new chapter on digital signal processing.


I got involved quite late in the project for this new chapter. The importance of digital signal processing in amateur radio has just kept on increasing as variable digital filters, adaptive noise reduction filters, adaptive notch filters, digital demodulation, and software defined receivers are everywhere.

The entire book project was handled by the Bergen group of the Assocation of Radio Amateurs in Norway. In fact it was done in order to celebrate their 90 year anniversary. The editor has been Frode Igland, LA6VQ.

My efforts resulted in a completely new chapter which was written during the first few months of this year. It was finalized with valuable input from the editor after a process of sending the manuscript back and forth lots of times. It was a fun project, where the challenge was to convey complex ideas with a minimum of equations.

The chapter has these headings:
  1. Applications of digital signal processing 
  2. Discrete values
  3. Quantization - digitization of amplitude
  4. Sampling - digitization of time
  • Aliasing
  • Nyquist frequency
  • Reconstruction filters
  • The time domain
  • The frequency domain
    • The Fourier transform
    • The Fast Fourier Transform (FFT)
  • Digital Filters
    • Moving average as an example of an FIR filter
    • IIR filter equivalent of a low pass RC-filter
    • IIR filter equivalent of a high pass CR-filter
  • Example of a software defined receiver with spectral display
  • The final section briefly discusses the RTL-SDR and uses an example from this blog showing activity of secondary users in the 70 cm band as shown here.

    So you want to play with a Pixie 2?

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    My own surface mount version of the Pixie2
    Here's a guide to Pixie 2 and related kits in a table format. These are minimalistic single-band transceivers which are fun to build, yet they perform well enough to be used, although with some effort, for real contacts.

    The idea of using the power amplifier transistor as a mixer seems to come from George Burt - GM3OXX - whose five transistor FOXX was described in 1983 in SPRAT. The basic design of the oscillator, PA/mixer and the simple keying has been more or less unchanged since RV3GM - Oleg Borodin - described the four transistor Micro-80 in 1992 in SPRAT. Later the Pixie 2 by WA6BOY replaced two of those transistors with the LM386 audio amplifier (QRPp 1995). Most later versions are variants of these designs.

    Here's the table of Foxx, Micro 80,  and Pixie2 kits:

    Foxx


    Foxx-3 kit from Kanga, £29.95
    Incorporates a sidetone oscillator, changeover relay and low-pass filter. Different versions for the 80, 40, 30 or 20 m bands

    Micro-80


    Kit from QRPme, $35.00
    Micro80D.
    Updated version with choice of  high or low impedance headphone, polyvaricon tuning cap and board mounted connectors, 80 m.

    Pixie2


    Kit from HSC Electronic Supply, $14.95
    For 80 and 40 m.
    Eham review

    Kit from Kenneke, $29.95
    Includes 80 m crystal

    Kit from QRPme, $40.00
    Lil Squall Transceiver ][.
    Several components and the output low pass filter are on sockets. Comes with a crystal for 40 m.

    Ali Express Ham QRP DIY Kit Shack 40 m, $15.07
    40 m version. Tuning pot for VXO.

    Radi0kit, £22.00
    Enhanced Pixie2 which comes in 80, 40 and 20 m versions. Judging from the PCB layout it has an improved pin 7 muting circuit.

    What can I say to characterize these designs? One the one hand they are very simple to build and get to work. One the other hand they are also simple in the sense that they do not always perform very well. Therefore I don't think I would recommend them to any novice ham. It takes some understanding of frequency offsets and sidebands in order to make real contacts.

    But lots of people have had great fun with such a minimalist transceiver which in its basic version puts out some 2-300 mW. And it encourages experimentation and modifications. Also, it should be remembered that it isn't really necessary to get a kit, as the Pixie 2 is quite simple to build from scratch also. I did that myself to try out surface mount technology.

    The original designs and many variants and modifications are documented in the Pixie file document of SPRAT. There are many, many more clever modifications out there and I have my share on this blog also. To sort out and link to all the other pages is too daunting a task, so therefore I have focused on kits here. Finally I wouldn't be surprised if the table is incomplete so I would appreciate comments if you think that something is missing.

    Milestone in blogging

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    Today the number of hits on my blog just exceeded a quarter of a million. When I converted my old web pages to a blog I didn't really expect this many readers, so I thank you all for each and every hit on one of my 106 blog posts.

    I have been blogging here since May 2011. But I have actually 23 posts which are older than that as I copied posts from my old web pages and gave them the original date of publication. The oldest post actually dates back to 2001 and is the first modification I published for my Elecraft K2. That was the year when I got my ham radio license

    These are the most popular posts:
    1. How to make a very cheap VHF receiver (2011)
    2. The best of the Baofeng handhelds (2013)
    3. QRPp: Ultra low power operation with the Pixie (2011)
    4. Scratchy Tivoli Model One (2013)
    5. Temperature compensation for an Arduino ultrasonic distance sensor (2014)
    6. A regenerative receiver for the 40 m band (2011)
    These pages (not posts) are also among the most popular ones:
    1. General modifications applicable to any Elecraft K2
    2. Unofficial Guide to Elecraft K2 Mod's
    One thing I have learnt is that hands-on articles are the more popular ones, and they don't necessarily have to be on ham radio topics.

    Congratulations to Logbook of the World

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    Congratulations to the ARRL Logbook of the World (LOTW) which just reached 100 million confirmed contacts. This is the same as an impressive 200 million QSL cards out of about 630 million uploaded contacts on LOTW.

    LOTW was established way back in 2003. This was only 2 years after I got my license. Since I have never enjoyed much to fill in QSL cards I embraced LOTW very quickly. I have to say though that I will of course respond with a paper QSL for those who ask for one.

    But LOTW has been my primary means of confirming contacts for a decade. My DXCC was confirmed with LOTW.

    Now at the same time that LOTW is celebrating 100 millions confirmations, I am celebrating 8 bands with 100 or more contacts all confirmed via Logbook of the World. This is on all bands from 3.5 to 28 MHz and has been my goal for many years. The last confirmation came from the TC0A contest station in Turkey on 80 m after last month's CQ World Wide CW contest.

    I consider myself lucky to have reached 100 confirmations even on the elusive 12 m band which we all know will shut down soon not to reopen again until the next solar maximum in about 11 years time.

    But as the saying goes "The journey is the reward", so what to do next as a radio amateur?




    Waiting for an AP510/AVRT5 APRS tracker

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    I just ordered an AP510/AVRT5 APRS tracker and am anxious to get my hands on it to try it out. I like the small size and the fact that it is self contained - no external wires are needed to have a fully functional tracker for the automatic packet reporting system APRS: But is it useful or just a toy?

    The specifications from the Amazon.co.uk site are (adapted from Chinglish):
    • SainSonic AVRT5 APRS Tracker VHF with GPS/Bluetooth/Thermometer/TF Card, Support of APRSdroid
    • GPS module: SIRF3 module, high sensitivity, fast positioning, stable power.
    • GPS antenna: 18mm x 18mm active GPS antenna, built-in LNA amplification, Star Search, locate quickly.
    • VHF Module (1W): The latest 1W VHF transceiver modules, small size, high stability for all types of wireless data transmission.
    • VHF antennas are individually matched to transmitter to ensure that the standing wave ratio is proper and the emission is efficient.
    I also signed up for the Yahoo group AP510 AVRT5 APRS.

    What attracted me were the reviews given by DK7XEDJ7OO (German), and APRS.facile.fr (French) and the descriptions at Radioddity and Sparky's blog,

    It is evident that the 2. harmonic suppression leaves something to be desired, that the antenna is inefficient, that the programming interface isn't the easiest to deal with, and that it can be hard to set the frequency for people in countries such as Norway with PC's set for "," rather than "." as the decimal point. Hopefully I can figure out ways to deal with all these and also other issues that may show up.

    Getting ready for 60 meter

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    I have never had any contacts on the 5 MHz or the 60 meter band. But I guess it's time for that now.

    Both my K2 and my K3 support it and about 40 countries now have access to this band according to K1ZZ in his column "It seems to us" in this month's QST.

    As a first test I ran my 0.2 W Ultimate 3 GPS-controlled WSPR transmitter over night and the image shows the result. I am using an 80 m long loop skywire antenna (horizontal loop) tuned to 60 m.

    The results were encouraging with the best DX being UR5VIB in Ukraine at a distance of 1887 km. By the way, considering that it is 1093 km to LA9JO in the north of Norway, one sees the distortion in the map projection used for the Google map.

    I have also operated the antenna as a vertical (about 8 meters) with top-hat loading by tying both feed-line conductors together and feeding it against a ground plane. The result is quite similar. The article by Dave Fischer, W0MHS called "The Loop Skywire" in QST November 1985 is the reference for both uses of the loop. The article starts out with this catchy phrase: Looking for an all-band HF antenna that is easy to construct, costs nearly nothing and works great DX? Try this one! This matches my experience exactly as this antenna has been instrumental for my 8 band DXCC.

    0.2 Watts to South Africa

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    This is a new one for me: Norway-South Africa on 30 m WSPR in the middle of the night. Again I am amazed at what this mode can accomplish, and also what my little Ultimate 3 kit is able to do. 

    The antenna used on my side was my trusty old 80 m long horizontal loop fed with a 4:1 balun and no tuning beyond that (SWR 7:1). Output power was from a single stage BS170 driven at 5 Volts, or about 200 mW in a 50 ohms load. In this particular antenna, the output is most likely much lower. 

    ZS6KN is the only non-European station who has heard me this night on 30 m, with a marginal SNR of -27 dB.


    - Hardly any young people are becoming hams anymore

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    This is what Ed Muns, W0YK, said in an interview the other day, and goes on with "because they see this as kind of old school stuff."

    A year ago the ARRL web site said: "Amateur Radio showing steady growth in the US". AH0A's website with statistics over the US ham population backs this up with the curve shown here. Even in my local club we are now seeing young people signing up for licence classes. 



    How different perspectives! How has an old radio amateur like W0YK come to believe in the myth of declining numbers of hams?

    Dimming my Ultrafire WF-501B

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    I got this red LED flashlight as a Christmas present. But unfortunately the intensity was way too high for what I intended to use it for. A soft red light preserves your night vision, and is ideal for use with a telescope in the dark as was my intention. But if the intensity was as high as before the modification, night vision would suffer anyway.

    I then found this YouTube video describing how the controller circuit board could be replaced by one with more functions. As recommended I therefore ordered an AMC7135*8 2800mA 4-Group 5-Mode Circuit Board with 8 AMC7135 current regulators in parallel. The image shows the original circuit board as connected before the modification in the front in the image and the new one behind it.

    The new board gave me the choice of one of 4-groups:
    1. 3-mode: Lo (5%) - Hi (100%) - Strobe
    2. 3-mode: Lo (5%) - Mid (30%) - Hi (100%)
    3. 2-mode: Lo (10%) - Hi (100%)
    4. 5-mode: Lo (5%) - Mid (30%) - Hi (100%) - Strobe - SOS
    I selected the second one by bridging the corresponding gap on the circuit board. The lamp will take either a single 3.6 Volt battery or two smaller ones in series which is what I had. Before the modification the LED lamp would consume 0.68 Amps from 2x3.6 Volt batteries. Now it consumes 0.14, 0.83, or 2.4 Amps. The controller remembers the last mode if the light stays off for more than 2 seconds. If the flashlight is turned on again faster than that it will change to the next mode. 

    I am very happy with the Low setting, but I wish I could have avoided the very power hungry High setting. I am not even sure if there is enough cooling for the LED and the controller to take that much current over a longer period of time. Perhaps a board with fewer AMC7135 chips would actually have been better, like this one with 3 rather than 8 chips and max current 1050 mA? Anyway, the whole modification took only 20 minutes or so.

    Finally got my Ultrafire WF-501B as I wanted it

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    As I wrote in my blog post a few days ago, I got the intensity down for night vision for my red flashlight. But I wasn't quite happy with the level and wanted to reduce it even more. To do that I had to unsolder 6 of the 8 AMC7135 350 mA constant current ICs on the PCB of the AMC7135*8 2800mA 4-Group 5-Mode Circuit Board.

    These constant current chips are all run in parallel with the VDD input for control. The 8-pin Atmel ATtiny13A chip controls all VDD inputs in parallel from its pin 6. When the VDD pin is low there will be no light. I haven't measured this, but I am assuming that this pin is pulsed in order to reduce current down from the maximum.

    My measurements for the High, Medium, and Low settings are:
    • 8 chips: 2,8 A, 0.83 A, 0.14 A
    • 4 chips: 1,4A, 0.45 A, 0.08 A 
    • 2 chips: 700 mA, 225 mA, 42 mA
    This scales as expected with the number of 350 mA chips and the 100%, 30%, and 5% settings of the controller. Now only Q1 and Q3 remain, and Q2, Q4-8 have been desoldered.

    One could have obtained en even more battery-friendly version if somehow the original controller could have been modified. The step-down circuit is quite standard with an inductor, a Shottky diode (SS14), and a controller chip of unknown origin. But it seems to me that if R23 of value R250 (0.25 ohm) was increased, output current would probably go down.

    As it is I am much more happy with the intensity of the settings I have now. It will be a good companion night light which will preserve night vision well when used with a telescope.

    Low power longwave transmitter experiment

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    Many places in the world, low power transmitters in the medium wave band are allowed. I am talking about regulations like in the US where FCC part 15 allows up to 100 mW input.

    In Norway we have a particular permission for members of the Norwegian Radio Historic Society to transmit up to 500 mW on 216 kHz in the longwave band. I'm not sure if this is output or input power [it's output power]. The permission is meant to cover a personal collection of historic radios. The frequency is the one used by the main transmitter north of Oslo from 1954-1995 running 200 kW. The frequency is still allocated to Norway, so I guess that is why we may use it this way.

    I grew up close to this transmitter and have fond memories of my first homemade crystal set receiving this station.

    There are several low power transmitters around that can be purchased, but most of them only cover the medium wave band and not longwave (153-279 kHz). Further they are quite complicated as the frequency necessarily has to be user settable.

    I looked for a simpler way to make a single-frequency transmitter and found that the function generator chip XR-2206 which I happened to have in my junk box could both generate this frequency and do the amplitude modulation. The RC-oscillator seems to be stable enough for this low frequency although I haven't tested this much.

    Here are the first results with images of the circuit on a Veroboard and the oscilloscope picture of the modulation with my Tandberg TP41 70's radio on top of it listening to Dire Straits from Spotify streaming over longwave.

    The circuit has very little output power, lacks antenna tuning and harmonic filtering, so there is room for improvement, but at least it works.

    Too bad that the XR-2206 is obsolete and not recommended for new development!


    All continents in one night on WSPR

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    For me South America, Australia, and Africa are quite rare on WSPR. But they all heard my tiny 0.2 W signal the night between 31 March and 1 April in addition to North America, Asia and Europe. That's a new one for me and worthy a brag post on the blog, I think! Hopefully, it may also inspire others to try low power WSPR.

    In Australia and South America I was heard on the 10 MHz band, in Africa on 21 MHz, in Pakistan on 14 MHz, while 7 and 10 MHz worked into Siberia. North American stations also heard me on the 7 and 10 MHz bands.

    This was on my untuned 80 m horizontal loop fed with open-wire feeder and a 4:1 balun. This shows both that the bare-foot Ultimate 3 kit is very tolerant of loads with SWR much different from 1, and that WSPR gives amazing results.

    Car upgrade to LEDs

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    It was time to upgrade the interior lights in my 2004 Volvo. I got some lamps from Ebay specified as 42 mm LED Festoon, 80-85lm, 12V. As many others have experienced also, they kept on glowing faintly after the door was closed. But when the ignition was turned off the lamps were completely off also, so there was no danger of draining the battery. Still this is not the way one expects lamps to behave.

    One can get more expensive LED lamps which avoid this faint glow, "Canbus error free" seems to be the way to specify this. But mine were of the plain type, and the problem seems to be the leakage current in the FET switches that turn the lights on and off. It is tiny, but enough to give a voltage large enough to turn the LEDs on. An additional resistor load will lower the voltage below that threshold.

    This requires a parallel resistor. Some have used 1k, others larger values. I did some trials and found that 10k worked well, while 22k didn't completely eliminate the faint glow. The advantage is that 10k will only dissipate 18 mW @13.5 Volts, while the 1k will dissipate ten times that. Therefore I could use a small 1/4 W type. I soldered it on the back of the LED-board as the image shows.

    The reason for switching to LED is not really to save energy as the savings aren't that great anyway. The whiter and brighter light is more important as you can see in the image with the LED to the left and the old incandescent lamp to the right.

    While at it, I just had to do some reverse engineering of the LED lamps. There seems to be four parallel groups of three series-connected LEDs (the three in a row) giving a forward voltage of about 8.3 V. They are driven via a resistor of 120 ohms in series with what seems to be a bridge rectifier since the lamps don't depend on being connected in a particular way with respect to polarity.

    In total it draws 18 mA @ 12V and 28 mA @ 13.5 V, i.e. 0.3-0.4 W, compared to 10 W for the bulb it replaced. This is not a very fancy way of constructing a LED lamp as there is no constant current regulation. The intensity will therefore vary with voltage, but hopefully it will work well here.

    A beauty of a crystal radio

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    This past weekend during Hammeeting - the largest Ham rally in Norway - I met Per LA9DTA.

    He showed me his beautiful crystal radio. It can be seen in the center of the table, with some close-ups below. The design has a printed coil and the whole design is made on a PCB which was shaped as shown in the image. It has a bandswitch and a Soviet low forward voltage Ge diode.

    I fell for his design, but with the lack of longwave and medium wave transmitters here I am not sure if I would have much use for it. That is unless I set up one of my transmitter projects to support a radio like this.

    I was demonstrating WSPR with my Ultimate 3 transmitter. It can be seen on the right hand side of the table. I wanted some fresh spots as I was giving a presentation later that day entitled "WSPR, JT65, JT9: Digital modes by Nobel laureates K1JT for HF DX with simple equipment". As I was spotted both on 40 m and 80 m I was happy with the performance. Per had also brought his Ultimate 3. Not the modified 11-band version, but just a plain one this time.

    First 475 kHz WSPR decoding

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    Tonight I made the first successful decoding of WSPR on the 630 m band. What inspired me was all the talk on the Elecraft reflector on the new synthesizer which in addition to having less phase noise, also allows the K3 to go below 500 kHz. I don't have that synthesizer, but the discussion reminded me of the low frequency converter I built many years ago. It converts 0-1 MHz to 14-15 MHz. Using the KXV3 transverter interface of the K3 it was easy to interface and get up and running.

    The first signals I decoded are shown in the water fall above, and their origin in Germany and the Netherlands is shown in the next figure.

    According to WSPRnet, PA0A's 2 Watt transmitter is 784 km away from me, and DK7FC's 1 Watt is 1164 km away.

    The converter is quite simple and is based on a 74HC4053 switch used as a mixer with a 74HC04 for a 14 MHz oscillator. It is the design of SM6LKM, but with a different oscillator frequency and a simplified output filter compared to his. It is one of many small projects that I have built in Altoids tins.

    The antenna used was my trusty old 80 meter horizontal loop which has been the main work horse for making my 8-band DXCC (all bands 3.5 - 28 MHz) possible. It is fed with ladderline into a 4:1 Elecraft balun in the shack.

    Perhaps the next step is to finish the 475 kHz filter of my Ultimate 3 WSPR transmitter and see if others can receive me? That is going to be more of a challenge antenna-wise.


    Ultimate software is up to date

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    As I have mentioned several times on this blog, I have thoroughly enjoyed WSPR modes ever since Hans, G0UPL came out with the first Ultimate QRSS/WSPR kit.

    That means that I have three different versions of the kit. Since Hans has kept on updating the software and even published the compiled versions, it is also possible to upgrade even the old ones.

    I have done that and the displays here show the Ultimate 3, the Ultimate 2, and the Ultimate 1 with the latest software.

    It is possible to upgrade the chips in-circuit, but I found that it is simpler to remove the chip temporarily from the socket and move it to a simple veroboard with crystal oscillator components. It is connected to my Ebay version of the USBtinyISP.




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