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I am always nervous about lightning strikes.

The excellent Southgate News today told the (true) story of a local CBer who had his vertical and CB rig destroyed by lightning. See http://www.huntspost.co.uk/news/latest-news/
huntingdon_cb_radio_user_almost_electrocuted_after_lightning_
bolt_strikes_aerial_1_3648368http://www.huntspost.co.uk/news/latest-news/
huntingdon_cb_radio_user_almost_electrocuted_after_lightning_
bolt_strikes_aerial_1_3648368

I usually disconnect antennas when there is lightning about but I am still nervous.  One of my friends (not a radio ham and with no big antennas in the air) who lived in a normal estate home had his home struck years ago and it took out lots of his household wiring. The chances of a direct hit are rare, but I am always bothered and never quite sure what the best advice is.

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 sheet	26 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:

• Dave Dilatush no-frills LM386 model.
• Comments on the quality of the LM386 Spice model.
• Datasheet for LM386

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 100 10uF
*rfeed nc3 100 {Rvar};     LTSPice
*.STEP param Rvar LIST 0.01 10Meg;          LTSpice

rfeed nc3 100 10Meg;     TopSPice
.STEP Rfeed LIST 0 10Meg;    TopSpice

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

.probe
.ac dec 100 10 1e6 ; 100 steps per decade from 10 Hz to 1 MHz
*.tran 1u 3m 0 5u
.save vdB(speaker)
*.print ac V(speaker);  LTSpice
.print ac vdB(speaker); TopSPice

vsupply vcc 0 dc 9
rsupply vcc vs 10
csupply vs 0 470uF

vsignal inn 0 ac 1 sin 0 .05 1k
rplus nc1 0 1e-6

* Output circuitry
csnub output snub .05uf
rsnub snub 0 10
ccoupling output speaker 250uf
rspeaker speaker 0 32

xamp inn nc1 nc2 nc3 nc4 output vs 0 lm386

cbypass nc2 0 0.1uf ;bypass cap for PSRR

************************************************************
* Bass boost (in LM386 Data Sheet)
.subckt BassBoost nc3 output
cfeed output 10 33nF
rfeed nc3 10 10k
.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:     2   3   7   1   8   5   6   4
*              |   |   |   |   |   |   |   |
.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 10013 10011 10008 ddpnp
q4 10014 10012 g1 ddpnp
r3 vs byp 15k
r4 byp 10008 15k
r5 10008 g8 150
r6 g8 g1 1.35k
r7 g1 out 15k

* input stage current mirror:

q5 10013 10013 gnd ddnpn
q6 10014 10013 gnd ddnpn

* voltage gain stage & rolloff cap:

q7 10017 10014 gnd ddnpn ; 
c1 10014 10017 15pf

* current mirror source for gain stage:

i1 10002 vs dc 5m  
q8 10004 10002 vs ddpnp
q9 10002 10002 vs ddpnp ; diode

* Sziklai-connected push-pull output stage:

q10 10018 10017 out ddpnp
q11 10004 10004 10009 ddnpn 100 ; diode D1
q12 10009 10009 10017 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-----------

We welcomed our second child, a daughter, into the family last week.  Since she is our second, the time in the hospital was more about making sure she was healthy than us learning all the ropes.  So, I had some undisturbed time to read on the Internet with a sleeping baby on my chest…and wish I could remote control my station.

Having been party to the discussion surrounding remoting a local contest station (K4VV), I had seen enough traffic about different VOIP options to start with Mumble for the audio stream.  I set up a Mumble server on my Linux server at the house, and then setup the Mumble client on my hamshack computer.  I ran a 1/8-inch TRS cable from the rear-apron line-out port of the K3 into the line input of one of my sound cards on the computer.  I put a free Mumble client on my iPhone and viola!  It worked out of the box.

I have been using Pignology’s HamLog on my phone for quick logging of one-off QSOs and goofing off with its vast array of tools.  HamLog also has the ability to remote control a rig using Pignology’s hardware.  Since, I’m really not in a good position to drop $300 on a box I’ll use a couple of times per year, I reasoned that there might be an alternative.  Enter the socat utility:

root@tula:~# socat /dev/ttyUSB1,raw,echo=0 tcp-listen:7373,fork

Freakin magic.  I used HamLog to connect to a “Remote PigTail” and it mostly works.  The frequency display does not seem to work and HamLog loses the connection if the phone falls asleep.  But, it is functional.  Another interesting wrinkle is that when my shack PC screensaver comes on, it mutes the audio stream piped into Mumble.  But, those are all minor irritations at this point considering the trivial amount of effort that went into getting a remote control going…

I decided to listen on the second pass of the new satellite deployments, this time using the Funcube Dongle Pro, recording in baseband, so I would have the chance to replay it again if there was anything interesting.

QB50P1 was heard sending CW, QB50P2 was sending QPSK. Down on the 145.865 there was some CW (a sample was B1UARJZB4K – hopefully not too many errors there!) which I think may have been Nanosat-BR

Fascinating!

With the launch of a number of Cubesats this evening, I was keen to take a listen on the first pass over the UK. I listened for QB50P1 on 145.815 and QB50P2 on 145.880. The pass was very low here – only a couple of degrees, but I was delighted to hear QB50P2 on CW – weak but easy copy.

You can read more about the satellites here

Latest TLEs for tracking here

On Twitter, Dave G4DPZ reported he’d heard P1, so they are both alive and well!

With limited space for antennas, it seems sensible to concentrate efforts on just a couple of bands only. As my favorite band is 10m, I am tempted to erect a more efficient antenna for this band and maybe put up the 6m V2000 only during the Es season. My problems are (a) a lack of mobility because of my stroke and (b) choice of compact, efficient antennas. At present I can cover 40, 20, 10, 6, 2 and 70cms, plus 630m rather inefficiently with my earth electrode antenna. Perhaps, whilst my health is not too good, I am better sticking with what I’ve got? I know that on 10m my antenna could be better but the Par end-fed covers 3 bands (10, 20 and 40m) and my 2W QRP has reached VK on WSPR on all these bands and doesn’t do a bad job.The Par is is almost impossible to see in the air.