AmateurRadio.com

I recently watched two superb YouTube videos. The first described exactly how to determine the 'shielded' side of a fixed capacitor and the importance of knowing this information.

As you have probably noticed, most modern fixed capacitors no longer indicate the 'grounded' end or the lead going to the internal shielding. At one time, the capacitor's polarity was commonly marked with a band on one end but this is no longer the case ... even though one side is indeed still the shielded side. Depending on exactly what part of the circuit your fixed capacitor is being used in, connecting it in the reverse direction (shield going to signal side), can introduce hum, RF pickup, instability and generally result in poorer capacitor / circuit performance ... and all it takes to determine which lead is which is an oscilloscope!


The second video I viewed shows the process used to resurrect a Yaesu FT-1000MP in truly terrible condition. In a very professional step-by-step process the video shows the logical and systematic approach at making the radio better than new.


Both videos are done by a truly gifted engineer, Paul Carlson, VE7ZWZ, and are exceptionally well done ... the quality one would expect to have to pay for rather than freely view on YouTube.

If you visit Paul's YouTube channel, you'll find a host of other radio and audio-related videos and I guarantee that you will learn something of value ... and probably hang around to watch several more. They are really well done.
Steve McDonald, VE7SL, is a regular contributor to AmateurRadio.com and writes from British Columbia, Canada. Contact him at [email protected].

Pofung UV-6R 136-174MHz & UHF:400-470MHz Dual Band Handheld FM Professional Two-way Radio

 

Lots of radio in a small package. Built well and performs well.

http://www.radioddity.com/

http://www.radioddity.com/skin/frontend/default/lanting/download/UV-6R%20User%20Manual

Brilliant Easy to read display

The first thing that impressed me aside from the size and quality was the brilliant and easy to read display of this radio. The two line display and the choice of display color make this radio easy to use and navigate through the menu system. The various option for screen color lighting also make the radio easy to read. The fact that the display lighting can be changed to suit the operator is a nice feature.

Superb audio quality

I have to say that after owning a few of the big 3 brand of radios I was thrown back by the outstanding and loud audio this radio has. I was not sure what to expect at first with such a small radio but the audio is outstanding, sounds great and no distortion even at full volume.

Features and Specifications:

• Dual Band Transceiver
• Brilliant L.C.D. Display
• D.C.S. and C.T.C.S.S. encoding
• VOX function
• Flashlight/Alarm feature
• FM radio band receive
• 128 memory channels
• Dual watch
• Menu driven programming
• Software available for programming (cable sold separately)
• Drop in Li-On charger
• 7.4v 1800mah Li-On battery
• High (5w) and Low (1w) power settings
• Accessory ports for adding speaker microphone (sold separately)
• Belt clip ( Soft case also sold separately)
• Selectable frequency steps
• Selectable repeater offsets
• Adjustable squelch via menu
• Adjustable TOT (Transmission Timer)
• Cross band receive/transmit
• Dual VFO
• Narrow and Wide FM selectable

And much more to even include in features.

The radio itself is great little performer. Battery life on receive is fantastic, battery life on transmit has yet to be determined. Looks rugged and fits nicely in the hand.

For the price of this radio (under $50.00 with free shipping to Canada and U.S.A.) you cannot go wrong for a radio to throw in your shirt pocket or your backpack as a take along radio to listen to N.O.A.A. weather stations, FM stations and monitor local repeaters. Accessories are all about one third each of the cost of the radio, which makes the low price of this radio even more impressive. The small antenna with SMA connector though lacks in receive performance of course, but other antennas can be purchased and used with this radio to get out of those fringe areas.

The Pofung UV-6R is a great introduction to the increasing line of radios on the market. It makes it affordable for the first time user and easy to operate; it also performs well and gets great audio reports into the repeaters. It’s light weight and long battery life make a great emergency radio for that go-kit or to have on hand when needed for that last minute hike.

Fred Lesnick

VE3FAL

**** (4 out of 5)

Fred Lesnick, VE3FAL, is a regular contributor to AmateurRadio.com and writes from Thunder Bay Ontario, Canada. Contact him at [email protected].

In this episode, Martin M1MRB / W9ICQ, Ed Durrant DD5LP ,Martin Rothwell M0SGL and Colin Butler M6BOY discuss the upcoming Ham Radio Friedrichshafen Event.

Colin Butler, M6BOY, is the host of the ICQ Podcast, a weekly radio show about Amateur Radio. Contact him at [email protected].

In this episode, Martin M1MRB / W9ICQ, Ed Durrant DD5LP ,Martin Rothwell M0SGL and Colin Butler M6BOY discuss the upcoming Ham Radio Friedrichshafen Event.

Colin Butler, M6BOY, is the host of the ICQ Podcast, a weekly radio show about Amateur Radio. Contact him at [email protected].

Here is this week’s space weather and geophysical report, issued 2015 Jun 22 0548 UTC.

Highlights of Solar and Geomagnetic Activity 15 – 21 June 2015

Solar activity was at low to moderate levels. Weak to mid-level C-class flares were observed on 15-17 Jun from Regions 2360 (N15, L=129, class/area Eac/220 on 12 Jun), 2367 (S20, L=002, class/area Ekc/400 on 15 Jun), 2268 (S06, L=100, class/area Bxo/010 on 14 Jun) and 2371 (N13, L=302, class/area Fkc/1180 on 21 Jun). Activity increased to moderate levels (R1-minor) on 18 Jun. Old Region 2365 (S13, L=079) produced a long duration event (LDE) M1 flare at 18/0127 UTC. At 18/1736 UTC, Region 2371 produced an M3/1n LDE with associated Type IV and Tenflare (2200 sfu) radio emissions. Associated with this event was an asymmetric, full-halo CME first visible in LASCO C2 imagery at 18/1724 UTC.

19 Jun saw a return to low levels with weak to high-level C-class flares observed from Region 2371. At about 19/0500 UTC, a large filament eruption was observed in the SSE quadrant of the disk. Associated with this eruption was a partial-halo CME, first observed in LASCO C2 imagery at 19/0845 UTC. Moderate levels returned on 20 Jun with an M1/if flare observed at 20/0648 UTC. 21 Jun saw a total of 4 M-class class flares. Region 2371 produced an M2/1n flare at 21/0142 UTC with associated Type II (682 km/s) and Type IV radio emissions. Also associated with this event was a full-halo CME. Shortly afterward, this same region produced an M2.6 x-ray event. At 21/0944 UTC, Region 2367 produced an M3/2b flare followed by an M1 x-ray event at 21/1820 UTC.

A pair of 10 MeV at greater than or equal to 10 pfu proton events were observed at geosynchronous orbit. The first event began at 18/1135 UTC, reached a maximum of 16 pfu at 18/1445 UTC and ended at 19/0230 UTC. This event was associated with the M1 flare from old Region 2365 observed at 18/0127 UTC. The second event began at 21/2035 UTC and reached at peak of near 50 pfu at the end of the summary period and was still rising. This event was associated with the M1 flare from Region 2367 observed at 21/1820 UTC.

The greater than 2 MeV electron flux at geosynchronous orbit reached high levels through the entire summary period.

Geomagnetic field activity was at quiet to active levels through the period. Quiet to unsettled levels were observed on 15-17 Jun with isolated active periods observed on 15 and 17 Jun. This activity was due to positive polarity coronal hole high speed stream (CH HSS) effects. Solar wind parameters, measured at the ACE satellite, indicated wind speeds of near 600 km/s early on 15 Jun decreasing to about 450 km/s by the end of the 17th. Total field ranged between 4-8 nT while the Bz component varied between +/- 5 nT. Phi angle was in a predominately positive (away) orientation. Predominately quiet conditions were observed on 18 Jun through late on 21 June. Solar wind speeds decreased from about 450 km/s early on 18 June to near 275 km/s by 21/1540 UTC. During this same time frame, total field ranged between 1-6 nT, Bz varied between +4 nT to -3 nT and phi remained mostly positive. After 21/1540 UTC, wind speed increased to about 360 km/s, Bt increased to 12 nT, Bz varied between +8 nT to -7 nT and phi briefly rotated to a negative (towards) sector. This deviation indicated a possible co-rotating interaction region in advance of an anticipated positive polarity CH HSS.

Forecast of Solar and Geomagnetic Activity 22 June – 18 July 2015

Solar activity is expected to be at moderate to high levels (R1-R2, minor-moderate). Active Regions 2367 and 2371, and the return of old Region 2365 on 30 Jun, are expected to keep activity levels enhanced through the outlook period.

The 10 MeV at greater than or equal to 10 pfu proton flux at geosynchronous orbit is expected to remain at the S1 (minor) to S2 (moderate) levels through 24 Jun. Effects from the 21 Jun M1 flare, coupled with multiple shocks from the 18, 19 and 21 Jun CMEs, are expected to keep proton flux above event levels.

The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal to moderate levels on 22 Jun through 06 Jul. Moderate to high levels are expected on 07-18 Jul due to CH HSS effects.

Geomagnetic field activity is expected to be at unsettled to severe storm levels (G1-G3, minor-strong) on 22-24 Jun. This activity is due to the expected arrival of the three CMEs from 18, 19 and 21 Jun. Unsettled to active periods are expected on 06-08 Jul, 12-13 Jul and 18 Jul, along with minor storm periods (G1-minor) on 05 and 11 Jul, due to CIR/CH HSS effects. Predominately quiet to unsettled levels are expected for the remainder of the outlook period.

Don’t forget to visit our live space weather and radio propagation web site, at: http://SunSpotWatch.com/

Live Aurora mapping is at http://aurora.sunspotwatch.com/

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As I write this on Sunday evening, June 21st, the magic band has been open here for over 16 hours straight and shows no signs of slowing down! What has been one of the poorest Sporadic-e seasons in memory, did not disappoint today, on what should theoretically be the peak day of the season.

A loud NØLL in Kansas was the first station heard this morning at around 0600 local time but I suspect the band had been open even earlier, judging by the strength of the signals. It didn't take long for the band to stretch out further and not too much later, signals from the Caribbean were making it into southern British Columbia, as well as many parts of North America.

At times the band seemed as crowded as 20m CW during the Sweepstakes as so many of the CW stations congregate in the 20KHz slot just below 50.100MHz. Before breakfast, the following stations were in the log:

        ZF1EJ Cayman Islands
          9Y4D Trinidad
          YV1KK Venezuela
          6Y5WJ Jamaica
          KP4EIT Puerto Rico
          XE2MVY Mexico
          XE2X Mexico
          WP3C Puerto Rico
          NP4BM Puerto Rico

courtesy: https://www.google.ca/maps

Around 10 am local time, the VA5MG beacon was suddenly heard pounding away ... often a good sign that propagation may be going 'polar'. Sure enough, stations to my south (Oregon and Washington) started to hear and work Europe. I was lucky enough to hear what can only be described as the contact of a lifetime, when K7CW (about 140 miles to the south) was heard working HVØA, the Vatican!! Paul was apparently in the sweet spot of the moment and his efficient homebrew array was up to the job. Over the next hour or so, the European propagation swung wildly between W7 and W6 as well as points to the east. The only Europeans that I heard were two Italian stations, briefly hitting 559 but unable to hear me. Johnny, KE7V (and also the brother of K7CW), about 40 miles to my south, managed to work both stations ... it seems that we were both just on the northern edge of the teasing footprint.

At times, several in band 'growly' carriers with polar flutter were heard as well as weak signals from some of the 49MHz videos still operating in central Europe.

It will be interesting to see if we have a repeat of this prop tomorrow (Monday) but I rather suspect much of this was the result of two well-placed solar flares earlier in the morning and will not be repeated ... I hope I'm wrong!

  Impact from the flares plus a slower moving one is expected later today.
Steve McDonald, VE7SL, is a regular contributor to AmateurRadio.com and writes from British Columbia, Canada. Contact him at [email protected].

OK, this is very low power but it shows you what can be done. A QRPP transmitter or signal generator anywhere between 500MHz and 1.5GHz.

Please note the image below is not on my blog (it is linked as shown) and will be immediately removed if this is a problem.

http://rtlsdrblog.rtlsdrblog.netdna-cdn.com/wp-content/uploads/2015/06/transmit_hack_rtlsdr-500×375.jpg

See http://www.rtl-sdr.com/using-the-rtl-sdr-as-a-transmitter/

See also http://www.steila.com/SDR/RFgenmod/index.html .

Roger Lapthorn, G3XBM, is a regular contributor to AmateurRadio.com and writes from Cambridge, England.