Like many of my projects, this transceiver is “on hold” due to my stroke. I am still too unwell to do much in the way of designing and building. One day, not too far away, I hope to complete this project. If anyone else wants to do this, please use my schematic as a starting point. With a small PCB it would make a nice club project.

It will make an ideal simple rig for nattering across town, especially as 10m loses its fizz and starts to act more like a vhf band again. Such conditions may be with us for years. I fancy putting this in a box like the old Heathkit Lunchboxes with a proper LS amp and LS.

See https://sites.google.com/site/g3xbmqrp3/hf/tenbox .

I wonder when the next round of price drops will come on Japanese gear? The big Japanese players such as Yaesu, Icom and Kenwood have had an easy ride of late and been able to dictate prices. Now the competition is waking up, I expect they will be facing tougher times.

The latest exchange rates (UK pound to Japanese Yen) is £1 is worth about 193 Yen. Not many years ago it was less than 130 Yen to the pound. In real terms, Japanese goods should be much less expensive. At the moment both the UK dealers and Japanese are doing very well thank you from a customer base prepared to pay high prices. Expect big falls between now and the year end. This will be partly due exchange rates becoming much better (for those in the UK) and partly due to the increasing threat from the non-Japanese suppliers. Don’t you find it amazing how low cost some Chinese hand portables are compared with similar products from Japan? Rip-off come to mind – charge high prices for Japanese goods as long as the suckers pay.

No, the age of UK amateur radio consumers being taken for a ride is ending. The next time you discuss prices with UK dealers remind them of competition and exchange rates! At the moment their margins must be very high. Japanese goods are priced too high in the UK – fact. A few years ago I was more sympathetic, but not any more. UK consumers should pay a fair price with the dealers getting a fair margin, but please don’t take us all for mugs. I shall buy when the prices are fair and not before.

If I have this wrong, I shall be interested to hear the dealers viewpoint. Exchange rates have got vastly better and I do not see this reflected in end user prices here in the UK.  Someone is making very handsome profits.

Consumers – vote with your wallets and do not buy overpriced radios.  I have said before, the FT817 is classic example: all development costs were recovered years ago, so the price should be considerably lower than it is. Dealers have dropped the price somewhat, but it is nowhere near what it should be for a very mature design.

Judy and I stopped by the Ashland Railroad Station today after visiting a blueberry field. I worked eight stations in the NA QSO Party and a station in Bulgaria. It was a gorgeous afternoon.

The station is one of the stops along the Plymouth and Lincoln Railroad that runs between Northfield and Lincoln, New Hampshire. The old depot is a museum now. The train makes regular stops there during the foliage season in the fall when the passengers disembark to tour the museum.

I tossed a 28 foot wire into a maple tree on the other side of the tracks and sat down on the platform with the KX3. I work part-time on the railroad as a conductor and know the train schedules.

The caboose in the background belongs to Brian, KA1JOZ who also works on the railroad. I started out on 20 meters. There were plenty of signals and the propagation was pretty good for a change. The North America QSO Party was in full swing and it was easy to make contacts. I seemed to have a pipeline to Minnesota. Here’s my log:

1 Aug-15 2011 14.019 NA0N CW 599 599 MN
1 Aug-15 2014 14.030 N0AT CW 599 599 MN
1 Aug-15 2016 14.033 N2UT CW 599 599 NM
1 Aug-15 2017 14.027 WO4O CW 599 599 Fl
1 Aug-15 2019 14.024 W9IU CW 599 599 IN
1 Aug-15 2020 14.019 K0MPS CW 599 599 MN
1 Aug-15 2021 14.018 K0AD CW 599 599 MN
1 Aug-15 2024 18.076 LZ73TRC CW 599 599 Bulgaria
1 Aug-15 2027 14.027 WA4PHC CW 599 599 NC

At one point I switched to 17 meters to see how the activity was. I heard LZ73TRC calling CQ. He was strong, and we had no trouble making a nice QSO. I operated for about 20 minutes and packed up.

Watch this video on a large screen. (It is HD). Discuss. Share.

This video features stunning clips of the Sun, captured by SDO from each of the five years since SDO’s deployment in 2010. In this movie, watch giant clouds of solar material hurled out into space, the dance of giant loops hovering in the corona, and huge sunspots growing and shrinking on the Sun’s surface.

April 21, 2015 marks the five-year anniversary of the Solar Dynamics Observatory (SDO) First Light press conference, where NASA revealed the first images taken by the spacecraft. Since then, SDO has captured amazingly stunning super-high-definition images in multiple wavelengths, revealing new science, and captivating views.

February 11, 2015 marks five years in space for NASA’s Solar Dynamics Observatory, which provides incredibly detailed images of the whole Sun 24 hours a day. February 11, 2010, was the day on which NASA launched an unprecedented solar observatory into space. The Solar Dynamics Observatory (SDO) flew up on an Atlas V rocket, carrying instruments that scientists hoped would revolutionize observations of the Sun.

Capturing an image more than once per second, SDO has provided an unprecedentedly clear picture of how massive explosions on the Sun grow and erupt. The imagery is also captivating, allowing one to watch the constant ballet of solar material through the sun’s atmosphere, the corona.

The imagery in this “highlight reel” provide us with examples of the kind of data that SDO provides to scientists. By watching the sun in different wavelengths (and therefore different temperatures, each “seen” at a particular wavelength that is invisible to the unaided eye) scientists can watch how material courses through the corona. SDO captures images of the Sun in 10 different wavelengths, each of which helps highlight a different temperature of solar material. Different temperatures can, in turn, show specific structures on the Sun such as solar flares or coronal loops, and help reveal what causes eruptions on the Sun, what heats the Sun’s atmosphere up to 1,000 times hotter than its surface, and why the Sun’s magnetic fields are constantly on the move.

Coronal loops are streams of solar material traveling up and down looping magnetic field lines). Solar flares are bursts of light, energy and X-rays. They can occur by themselves or can be accompanied by what’s called a coronal mass ejection, or CME, in which a giant cloud of solar material erupts off the Sun, achieves escape velocity and heads off into space.

This movie shows examples of x-ray flares, coronal mass ejections, prominence eruptions when masses of solar material leap off the Sun, much like CMEs. The movie also shows sunspot groups on the solar surface. One of these sunspot groups, a magnetically strong and complex region appearing in mid-January 2014, was one of the largest in nine years as well as a torrent of intense solar flares. In this case, the Sun produced only flares and no CMEs, which, while not unheard of, is somewhat unusual for flares of that size. Scientists are looking at that data now to see if they can determine what circumstances might have led to flares eruptions alone.

Scientists study these images to better understand the complex electromagnetic system causing the constant movement on the sun, which can ultimately have an effect closer to Earth, too: Flares and another type of solar explosion called coronal mass ejections can sometimes disrupt technology in space as well as on Earth (disrupting shortwave communication, stressing power grids, and more). Additionally, studying our closest star is one way of learning about other stars in the galaxy.

Goddard built, operates and manages the SDO spacecraft for NASA’s Science Mission Directorate in Washington, D.C. SDO is the first mission of NASA’s Living with a Star Program. The program’s goal is to develop the scientific understanding necessary to address those aspects of the sun-Earth system that directly affect our lives and society.

https://www.youtube.com/watch?v=zXN-MdoGM9g

Watch this amazing explosion on the Sun. From sunspot complex 1226-1227 comes an X-ray Flare peaking at a magnitude of M2.5 at 0640 UTC on 7 June, 2011.

Source: https://www.youtube.com/watch?v=KQMrRu8BWDo

This X-ray flare hurled a massive coronal mass ejection (CME) toward the Earth. This not-squarely Earth-directed CME is moving at 1400 km/s according to NASA models. The CME did not deliver even a noticeable glancing blow to Earth’s magnetic field late June 8th or June 9th.

What can be seen clearly in this movie is one of the most spectacular prominence eruptions ever observed. In fact, one could call it a “prominence explosion”. The prominence material expanded to a volume some 75 times as big across as the earth!

This X-ray flare also triggered an S1-level solar radiation storm, causing a long-lasting polar cap absorption (PCA) event. A polar cap absorption (PCA) event affects the propagation of a shortwave radio signal as it makes its way over the polar regions. In short, radio communications on lower shortwave radio frequencies become more difficult, as those radio signals are absorbed by the ionosphere (in the D-region) over the polar regions.

What does this mean in real-world communications? Trans-polar airline pilots may find it more difficult to communicate with regional air traffic control, shortwave radio listeners who want to hear a broadcast from a country by receiving a transmission from a country by way of a transmission beamed over the pole (like, from Europe into the USA via the North Pole), or other such communications, will find those signals all but gone. The stronger the PCA event, the higher the frequencies absorbed over the polar regions, with the greatest absorption occurring at the lower frequencies.

This movie spans the period of time from 0300 UTC through 1556 UTC, and is composed of the 171-Angstrom, 304-Angstrom, and 335-Angstrom wavelength views as captured by the filters of the Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA). In this movie, the AIA instruments capture the Sun’s extreme ultraviolet light and reveal 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.

The following is a linked video that is part of this event: http://www.youtube.com/watch?v=L4CsjcUGoaw

Watch as we zoom out to see a total view of the June 7, 2011 moderately-powerful X-ray Flare and Prominence Eruption. This movie will give you a full perspective of the immense size of this prominence eruption as it spews out away from the Sun.

The X-ray Flare peaked at a moderate magnitude of M2.5 at 0640 UTC, but unleashed a huge prominence eruption. The massive cloud of plasma was ejected out into interplanetary space, but missed the Earth. This movie stars with a “close-up” view by the Solar Dynamics Observatory at a combined wavelength view at 94 and 304 Angstroms. Then, the movie views the event further back through the eyes of the COR1 spacecraft (with the SDO AIA 304 image superimposed in the middle). Next, we zoom out to the COR2 spacecraft and superimpose the COR1 and SDO views. Then, we zoom further back to the H1 view… and finally look again at the event close-up.

More info: http://sunspotwatch.com/

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Source: SDO AIA NASA SOHO

Stories you’ll find in our August, 2015 issue:

HF Air Monitoring: Understanding NOTAM Information
By Tony Roper

International air-route safety is everyone’s concern, no more so than with those who use the world’s air space daily—military, commercial and civilian aircraft. To help, the world’s aviation authorities make available Notice to Airmen (NOTAM) widely available. These notices tell all pilots what to expect along their regular routes across oceans and continents. But, they also give clues to air monitoring enthusiasts as to what type of aircraft may be in the air and on the air. Tony explains how to unravel NOTAM information to learn when and where to listen.

TSM Reviews: Whistler WS-1080 P-25 Phase I and II Scanner
By Chris Parris

The last few years have been revolutionary for the world scanning radios. In additional to the great technical strides that the manufacturers have pushed to the electronics market, some names in the scanner world have disappeared and new names have come to the forefront. One name new to the world of scanning is Whistler, of Bentonville, Arkansas. Prior to this, Whistler had previously been known for their line of radar detectors, GPS devices and power inverters, but no scanners. Chris takes a close look at this very capable scanner.

Advanced Radio Noise Filtering using DSP
By Geir Laastad LA6LU

Using the signal of a Norwegian Non-directional Aeronautical Beacon (NDB) Geir shows us how it is possible, in some cases, to achieve almost 100 percent noise-free radio reception with advanced use of Digital Signal Processing (DSP) technology. Using a combination of built-in filters and outboard DSP speakers, Geir describes techniques that are most effective for narrow band CW reception, but will also improve the reception of SSB or AM signals.

Digitally Speaking: Digital Voices on HF Part 1
By Cory GB Sickles WA3UVV

When most hams think of digital voice operation, they think of VHF and UHF repeaters. To be sure, that covers where the vast majority of digital voice QSOs take place. While simplex 2-meter and 70-cm activity is out there, in most areas it subsides once one or two repeaters are established in a given area. But, there are plenty of frequencies on HF where proponents of each digital methodology have established a foothold. Cory tells us where those frequencies are and what you need to get on the air.

Multiple Satellite Reception from a Single Ku-Band Dish (Part 2)
By Mike Kohl

Last month Mike walked us through the theory behind multiple feed horns on a stationary Ku-band dish for reception of Free-to-Air satellite signals. In Part 2 he shows how it’s done; crowding as many as 12 feed horns on one 1.8-meter Ku-band satellite dish that can see 12 satellites positioned from 89 degrees West to 119 degrees West. It requires making a custom feed support and takes meticulous adjustment to get it all right, but so worth it!

Scanning America By Dan Veenaman
Scanning Wisconsin; FCC Field Office Shuffle

Federal Wavelengths By Chris Parris
US Navy HYDRA Systems

Utility Planet By Hugh Stegman NV6H
What’s up with SKYKING?

Digital HF: Intercept and Analyze By Mike Chace-Ortiz AB1TZ/G6DHU
Irish Navy HF Operations

HF Utility Logs By Mike Chace-Ortiz and Hugh Stegman

Amateur Radio Insights By Kirk Kleinschmidt NT0Z
Gensets and UPSs: Play it Smart!

Radio 101 By Ken Reitz KS4ZR
2015 Field Day Report and the C64 Today

Radio Propagation By Tomas Hood NW7US
Sunspots Got You Down? You Can Still Work the World

The World of Shortwave Listening By Robert Wagner VK3VBW
Radio Verdad – Small Voice, Big Heart

The Shortwave Listener By Fred Waterer
Kid’s Shows, BBCWS and CRI

Amateur Radio Astronomy By Stan Nelson KB5VL
Noise in Radio Astronomy

The Longwave Zone By Kevin O’Hern Carey WB2QMY
You Have Questions…

Adventures in Radio Restoration By Rich Post KB8TAD
A Classic Pair of Heathkit Hi-Fi Twins
Part 1: the AJ-11 Tuner

The Broadcast Tower By Doug Smith W9WI
What Happened to WOWO

Antenna Connections By Dan Farber AC0LW
Soldiering on after a Microburst

The Spectrum Monitor is available in PDF format which can be read on any desktop, laptop, iPad®, Kindle® Fire, or other device capable of opening a PDF file. Annual subscription (12 issues, beginning with the January 2015 issue) is $24. Individual monthly issues are available for $3 each.