Posts Tagged ‘JT65’

Current set-up for WSPR, JT65 and JT9-1

This is a photo of the kit currently used. The top FT817ND is used mainly for 2m and 70cms (local FM net, SSB and CW, beacon hunting) and the lower FT817 for WSPR, JT65 and JT9-1 mainly on 6m and 10m. The lower rig is set at 2.5W, but the cable run to the V2000 vertical is lossy on 6m. I use a SignaLink USB audio interface to the PC.  This works well. For all digital modes I use the FT817 on DIG setting via the rear connector.   Sometimes I use the Z817 ATU, which I find very good. With this, I can get onto 5MHz and some other bands.

Best DX (on WSPR) is Australia at 1W out on 40, 20 and 10m and Israel on 6m WSPR (1W ERP).

Not shown (on shelf above) is the 472kHz homebrew transverter, the 15m MFJ Cub and the Mizuho 200mW 2m SSB rig. Also out of sight are a 136kHz beacon, the 2m Fredbox, the 6m Sixbox, the VLF 8-9kHz beacon, and optical rigs. I am waiting for better health to be able to use these again. Currently my operating is all from home and mainly modes not requiring me to talk, although I have ventured onto our Monday night FM net and the odd 2m and 70cm contest.

Same callsigns?

One of the drawbacks of WSPR (currently) is you tend to get spotted, or spot, the same stations over and over again. I am even seeing the same stations being spotted on 10m and on 6m.

It would be very nice if there were a lot more active stations, so spots came from a variety of stations. I am even seeing this on JT65 and JT9-1.

Perhaps people think these “new fangled” digital modes are hard and so only a limited number of people (currently) use them. Let me say, if even I can use these modes then anyone can! All these modes are great with low power and have really opened my eyes as to how far very low powered signal can be detected.

10m unique WSPR spots this afternoon (duplicates not shown)

Near miss – 11742km on 10m JT65

This evening CA3SOC (Chile) was calling CQ on 10m JT65. I called and called him – he called CQ about 14 times – but I was unable to raise him. At the start he was -16dB S/N but in the end was down to -22dB S/N. I was copied in Sweden at the same time, but that was no compensation.

Earlier in the afternoon I worked an E74 on PSK63, my first ever QSO on PSK at that speed. I am finding real-time keyboard operating in PSK modes quite “challenging”.  Whenever I use the keyboard e.g to write this blog, I make lots of errors that need correcting. This is hard on PSK31 and PSK63 in real time.   JT65 and JT9-1 are a lot easier. Currently I am using Digipan software which is simple and basic for PSK modes. I am using WSJTX V1.3 r3673 for JT65 and JT9-1.

Continuing JT65/JT9 today

When we get back from shopping I shall return to JT65-HF and JT9-1 modes hoping to work more stations. Yesterday, staying on 20m, I worked 4 Europeans running 2.5 or 5W. JT65-HF is very intuitive and works well. Althought I have had JT9-1 QSOs on 10m in the past, I suspect the rig stability is “challenging” and JT65-HF gives me a better chance. JT65-HF is some 4dB worse than WSPR but the TX period is only 48 secs (1 minute TX period but actual TX is less) so may be better with QSB?  JT9-1 is a narrower bandwidth mode than JT65-HF and is about 2dB worse than WSPR. Of course, JT65 and JT9 are proper QSO modes.

Sunspot count today is 76 (decent) and 20-30MHz conditions are supposed to be “normal” so there could well be some F2 (as well as Es) on 10m today. JT65-HF and JT9-1 on 10m are calling I think.

The great advantage of WSPR is you can set the rig running and monitor things in another room. JT65 and JT9 seem to require “hands on” operation, which is fine.

Been a busy boy

Been very busy with the day job and too busy playing radio so this post will be a bit of a catch up!

JT-65HF
I have been using my newly built datamode interface in anger.

As well as running WSPR on occasion I have also been active using JT65-HF.

JT65 is a communication mode developed by Joe Taylor, K1JT, (specification here) originally intended for amateur radio communication with extremely weak signals such as Earth-Moon-Earth (EME) contacts on VHF it has gained popularity on the short wave bands using JT65-HF an adaptation of the JT65A protocol.

Being restricted to 10W it is an attractive method of making contacts. The protocol includes error-correcting features that make it usable even when the signals are too weak to be heard or are being subject to interference.

There are several how-to guides available
Get On the Air with HF Digital (from the ARRL)
JT65-HF -- an 'Odd' but Fun Digital Mode (from eham.net)

A number of software packages support JT65, the most popular being JT65-HF originally developed by Joe, W6CQZ. Sadly Joe is no longer developing the software, but the last version released still works, and is available at http://sourceforge.net/projects/jt65-hf/ 

Thankfully the project was open source and Beat Oehrli, HB9HQX as developed his own version with the catchy title JT65-HF-HB9HQX-Edition, available at http://sourceforge.net/projects/jt65hfhb9hqxedi/ This is the version I have been using with great success, the colour coding and simple button pressing makes a QSO straight forward and the built in logging and exporting make uploading to QRZ, eQSL and HRDlog painless.

Whilst to a traditionalist amateur operator it is perhaps a little slow, remote and impersonal (each exchange occurs during alternate minutes) I really like it! One advantage is I can set up the radio in the shack with CAT control via HRD and then have QSOs while VNC'ing into the computer from the laptop whilst in front of the TV with the wife and the dogs! (Thanks Tim G4VXE for that suggestion!)

I have been active on the 10/20/30 and 40M bands over the past few weeks making contacts with Bulgaria, Canada, Denmark, Germany, Greece, Iceland, Kazakhstan, Poland, Russia, Serbia, Sweden, Thailand, Ukraine, USA and Venezuela.

Contesting 'DX' Headset and Interface

I have become hooked on the RSGB UKAC VHF contests, operating on a Tuesday evening on different frequencies (50MHz, 144MHz, 432MHz depending on which week of the month) Whilst my results are small-fry compared to the big guns I have been more than happy with my modest antenna set up and less than ideal location (previous blog posts)

I soon appreciated that using headphones rather than the speaker made life easier but I was still using the stock supplied hand microphone. Several times I have found it difficult to make myself understood and suspected that not only am I plagued by my 'Black Country' accent and poor enunciation but maybe the microphone wasn't quite cutting it.

Not able to afford or justify the purchase of a Heil headset just yet I took inspiration from Charlie M0PZT and his recommendation for a budget solution using a £10 computer headset from CPC (product AV21444).

On the Yaesu FT-857D the microphone connector is a 8-pin RJ45 socket which is behind the removable front panel with the lead coming out of one of a number of openings. Whilst the panel is easily removable I didn't want to keep removing it when switching between microphones, also re-purposing an obvious CAT5 network lead was problematic as they are often thicker than the openings.

The lead removed from MH-31, RJ45 on interface
A quick look at the supplied Yaesu MH-31 microphone revealed it can be unplugged, so what I needed was a interface box where I could plug in the headset and the microphone lead. This would also allow me to try different headsets in the future.

Mic lead connected and headset
The budget 'dx' headset
My solution as pictured above is quite simple, I won't include any pictures of the interior as it is a bit messy and not my best work! It is built from salvaged parts, including the box. The RJ45 socket came from an old network adapter, but beware some sockets are only 6 pin not the 8 as needed here. The headphone part of the headset is a simple connection to the rear socket on the FT-857D (the grey cable on the picture above)
Yaesu FT-857D mic socket as view from front
Most microphones designed for computers use electret elements which require a bias voltage, this is quite simple as the Yaesu microphone connector supplies 5V, so a simple resistor (8.2K) will supply this, also by using a couple of different capacitors and a switch I can select a 'thin' higher frequency response (for DX work) or a more normal 'fatter' response. A circuit can be found on George Smart's webpage, the bias is simply applied to the tip of the microphone jack.

The box also has a PTT switch, this could have simply grounded the PTT line but I wanted to have a LED indication on the box and again I could have just wired a LED and resistor to 5V and to the PTT line so it would light when the switch was closed, pulling PTT to ground and completing the circuit. I opted to use a simple transistor open collector switch to add a little isolation.

The interface works well and I used it for the first time last night in the 50MHz UKAC with my homebrew MOXON antenna...

6M/50MHz MOXON
My first contest back in January was the 50MHz UKAC and as I blogged I made a solitary contact due to antenna issues, i.e I didn't really have one!

I missed the February contest so this month I really wanted to have a decent stab at it which meant building an antenna. I decided early on that a Moxon was probably the easiest to construct, so I downloaded the MoxGen program to calculate the element lengths.

Using 1mm diameter 'garden wire' for the driven element and reflector. I had various bits of flexible plastic pipe kicking about and decided to use them to construct an x-shaped spreader, unfortunately the pipe was obviously from different batches and as soon as it was tensioned by the wire it bent into all sorts of strange shapes due to the different elastic properties so I abandoned that design.

I had left the build to the last minute and needed a quick solution, so yesterday morning plan-B was to go an get some cheap timber from the local B&Q on the way to work and build a simple frame to wrap the wire round.
Moxon on garage floor
Coax and common-mode choke, and sturdy support!
I impressed myself by completing the construction of the frame in the short time I had at lunchtime!

One thing I hadn't appreciated was just how big the final antenna was, it wasn't heavy just big! So last night an hour before the contest started I fitted the choke balun and coax to the terminal block. To be safe I removed the other antenna from the mast and hoisted her up.
Up in the night sky

Moment of truth, thankfully the VSWR was around 1.5:1 at 50.2MHz, rising to nearer 2:1 at the top end of the band. Not ideal but close enough. The VSWR measurements would suggest that the Moxon is a little bit long, interestingly some online Moxon calculators suggested dimensions for a slightly smaller Moxon than the downloaded Moxgen program did? Something to tweak/experiment with possibly using some thicker wire to increase the bandwidth.


50MHZ UKAC 25 March 2014
I was sorted! Moxon antenna up, contesting headset and interface plugged in and a quick scan up and down and I could clearly hear several stations testing and setting up. I poured myself a beer and soon the contest started.

Time between QSOs for a 'selfie'
I finished the night with just 14 QSOs, more would have been nice and it wasn't through lack of trying I could hear many more operators but simply couldn't make myself heard either because the antenna was in wrong direction or due to low power and getting lost in the pile ups to stronger stations.

I was not disappointed in fact I was quite happy with what my 10W, my new headset and home brewed antenna had achieved. The Moxon showed great promise and directional characteristics but for some reason just couldn't get south as the map indicates.


Out of interest I wondered what the line of slight view from my mast looked like so I strapped a camera on to the moxon this afternoon..


Need more height I think, especially if pointing South and a rotator would be nice!
Well that wraps it up for the moment.. 73

An Amazing Moment in Space Weather – Massive Solar Eruption June 2011

While many are talking about how Solar Cycle 24 is the weakest since the Maunder Minimum (the period starting in about 1645 and continuing to about 1715 when sunspots became exceedingly rare, as noted by solar observers of the time — see this Wiki entry), there are moments when activity on the Sun strongly increases, providing brief moments of excitement.

Here is a case in point, witnessed by the Solar Dynamics Observatory (SDO; see SDO Mission) on June 7, 2011, when the Sun unleashed a magnitude M2 (a medium-sized) solar flare with a spectacular coronal mass ejection (CME). The large cloud of particles mushroomed up and fell back down looking as if it covered an area almost half the solar surface.

SDO observed the flare’s peak at 1:41 AM ET. SDO recorded these images in extreme ultraviolet light that show a very large eruption of cool gas. It is somewhat unique because at many places in the eruption there seems to be even cooler material — at temperatures less than 80,000 K.

This video uses the full-resolution 4096 x 4096 pixel images at a one minute time cadence to provide the highest quality, finest detail version possible.  The color is artificial, as the actual images are capturing Extreme Ultraviolet light.

It is interesting to compare the event in different wavelengths because they each see different temperatures of plasma.

Credit: NASA SDO / Goddard Space Flight Center

Video: http://g.nw7us.us/1aOjmgA – Massive Solar Eruption Close-up (2011-06-07 – NASA SDO)

Visit: SunSpotWatch.com

 

Overmodulated JT65 on HF?

Sometimes it is crowded on JT65 on HF due to too little bandwidth. When only 2 kHz is available and each signal needs 175 Hz that’s understandable. But then others seem to complain that some overmodulate their transmitters so that they occupy more than the 175 Hz, making it even harder to fit an extra signal in the band.

As I have been running a lot of JT65 lately on HF, I also have seen this phenomenon and it pickled my interest to try to understand what was going on. The image below shows such a strong station to the very left, at about -1000 Hz where the red marker is located. After some seconds I turned on the attenuator of my K3, so the signal was attenuated by 10 dB (press image for zoom).
What one can see is that what appears initially (at the bottom of the waterfall) as a splattering signal, becomes quite fine when the attenuator is turned on. Then it spills into neighboring frequencies again as the attenuator is turned off again.
It appears then that it is the JT65 decoder software which is too sensitive to strong signals. Now, I cannot really say that I understand all of the decoder code, but I think that it has to do with the way the power spectrum is estimated. The FORTRAN code for ps.f is listed below. It comes from the BerliOS repository for WSJT which has the same code for this routine as JT65-HF-Comfort:
subroutine ps(dat,nfft,s)

      parameter (NMAX=16384+2)
      parameter (NHMAX=NMAX/2-1)
      real dat(nfft)
      real s(NHMAX)
      real x(NMAX)
      complex c(0:NHMAX)
      equivalence (x,c)

      nh=nfft/2
      do i=1,nfft
         x(i)=dat(i)/128.0       !### Why 128 ??
      enddo

      call xfft(x,nfft)
      fac=1.0/nfft
      do i=1,nh
         s(i)=fac*(real(c(i))**2 + aimag(c(i))**2)
      enddo

      return
      end

What is apparent here is that the raw data, dat, is just put directly into the Fast Fourier Transform routine, xfft, after scaling. There is no windowing function. A window function tapers down the beginning and end of the data set. Window functions in spectral analysis are somewhat involved and I refer to the Wikipedia article for details. But when there is no window function (= rectangular window), the first sidelobe is only 13 dB down from the mainlobe. So that could be why a 10 dB attenuator is enough to remove most of the spillover into adjacent frequencies above. 

This could be remedied by using a smooth window function. There are many to chose from, but let’s take a Hamming window as an example, with its first sidelobe 43 dB down. This means that if the data had been multiplied by this taper, the dynamic range would  have been in the order of 30 dB higher. But as data is lost by the tapering, the downside is that the bin width increases. For this particular window the noise bandwidth goes up by a factor of 1.36 so sensitivity would suffer by 10log(1.36) or about 1.3 dB (ref: Harris, “On the use of Windows for Harmonic Analysis with the Discrete Fourier Transform,” Proc. IEEE, 1978)There could potentially be other negative side effects on decoding also which I cannot foresee from the limited  time I have used in trying to understand the algorithms. 

My first impression from using the new JT9 mode is that the problem is much smaller there than for JT65, so maybe something like what I am discussing here has been done in the decoder software. But as far as I know, the source code has not been releasted into the public domain yet by K1JT, so I cannot verify it now.

But it seems clear to me that what looks like splatter has much less to do with overdriving and overmodulating transmitters than one may think, and more to do with the particular way that the spectral estimate is found in the JT65 decoder software. Combined with the variable propagation which is an intrinsic feature of HF and which may create a highly variable signal strength, this is what seems to create the spillover.


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