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Tuesday, April 21, 2026
The REALLY BIG Dish: China's Sky Eye
Tuesday, December 2, 2025
Grote Reber -- W9GFZ -- Radio Astonomy Pioneer, Homebrew Hero
Second, Grote Reber's mother was also the teacher of Edwin Hubble. Hubble was the guy who discovered that there were OTHER GALAXIES in the universe, and that they were all moving away from each other. That was a BIG discovery! Later, Grote's mom also had her son in her class. Both students were from Wheaton, Illinois.
Lest there be any doubt about Grote's dedication to radio, consider the following. (Much of the following comes from Wikipedia. https://en.wikipedia.org/wiki/Grote_Reber)
When he learned of Karl Jansky's work in 1933,[5][6][7] Grote Reber decided this was the field he wanted to work in, and applied to Bell Labs, where Jansky was working.
Pioneer of Radio astronomy

In the summer of 1937, Reber decided to build his own radio telescope in his back yard in Wheaton, Illinois. Reber's radio telescope was considerably more advanced than Jansky's, and consisted of a parabolic sheet metal dish 9 meters in diameter, focusing to a radio receiver 8 meters above the dish. The entire assembly was mounted on a tilting stand, allowing it to be pointed in various directions, though not turned. The telescope was completed in September 1937.[8][9]
Here is a really great article from Sky and Telescope magazine (July 1988) about Reber's homebrew radio telescope:
http://jump.cv.nrao.edu/dbtw-wpd/Textbase/Documents/grncr071988a.pdf
He was limited by the size of locally available 2X4 lumber. Neighbors thought he was trying to control the weather or to bring down enemy aircraft. Between Wheaton and the NRAO site in West Virginia, Reber's telescope spent some time at the National Bureau of Standards site in Sterling, Virginia. I was in Sterling just yesterday. I wonder if there is a plaque or something noting the telesccope's stay in that town. I note that at age 15, Reber had built a ham radio transceiver.
AND THEN HE MOVED TO TASMANIA
He did this because of propagation and low noise conditions. (This reminds me of how we sometimes said that very few people have actually said the words, "And then we moved to the Azores.")
Starting in 1951, he received generous support from the Research Corporation in New York, and moved to Hawaii.[12] In the 1950s, he wanted to return to active studies but much of the field was already filled with very large and expensive instruments. Instead he turned to a field that was being largely ignored, that of medium frequency (hectometre) radio signals in the 0.5–3 MHz range, around the AM broadcast bands. However, signals with frequencies below 30 MHz are reflected by an ionized layer in the Earth's atmosphere called the ionosphere. In 1954, Reber moved to Tasmania,[12] the southernmost state of Australia, where he worked with Bill Ellis at the University of Tasmania.[13] There, on very cold, long, winter nights the ionosphere would, after many hours shielded from the Sun's radiation by the bulk of the Earth, 'quieten' and de-ionize, allowing the longer radio waves into his antenna array. Reber described this as being a "fortuitous situation". Tasmania also offered low levels of man-made radio noise, which permitted reception of the faint signals from outer space.
His Homebrew House in Tasmania
In the 1960s, he had an array of dipoles set up on the sheep grazing property of Dennistoun, about 7.5 km (5 miles) northeast of the town of Bothwell, Tasmania, where he lived in a house of his own design and construction he decided to build after he purchased a job lot of coach bolts at a local auction. He imported 4x8 douglas fir beams directly from a sawmill in Oregon, and then high technology double glazed window panes, also from the US. The bolts held the house together. The window panes formed a north facing passive solar wall, heating mat black painted, dimpled copper sheets, from which the warmed air rose by convection. The interior walls were lined with reflective rippled aluminium foil. The house was so well thermally insulated that the oven in the kitchen was nearly unusable because the heat from it, unable to escape, would raise the temperature of the room to over 50 °C (120 °F). His house was never completely finished. It was meant to have a passive heat storage device, in the form of a thermally insulated pit full of dolerite rocks, underneath, but although his mind was sharp, his body started to fail him in his later years, and he was never able to move the rocks. He was fascinated by mirrors and had at least one in every room.
To Canada -- And a Rejection of the Big Bang
The same July 1988 issue of Sky and Telescope magazine has a good historical vignette of Reber, with a focus on his actvities in Canada late in life (click on the image below). Reber had big doubts about the big bang. Unfortunately this seemed to spill over into scorn and ridicule for those who -- well -- believed in the big bang. We see this at the end of the article. Oh well, even great people sometimes get cranky.
Three cheers for Grote Reber.
Monday, December 1, 2025
Book Review: "Big Ear Two -- Listening for Other-Worlds" by John Kraus (1995)
This book is kind of weird, but give it a chance. The author seems too prone to describe the physical attributes of his colleagues, especially female colleagues. But he was born in 1910 -- he was an old guy when he wrote this book, so perhaps we should cut him some slack. And there is one memorable episode where he defends a female applicant. In spite of the shortcomings, there are many real gems in there, often hidden among the descriptions of 1930's era Kleenex machines and refrigerators. I picked up the book a long time ago and only read it recently.
Here is a good review of Kraus's "Big Ear Two" book:
https://reeve.com/Documents/Book%20Reviews/Reeve_Book%20Review-Big%20Ear%20Two.pdf
Thursday, November 6, 2025
A Visit to the U.S. National Radio Astronomy Observatory (and the surrounding Quiet Zone)
Saturday, October 4, 2025
Monday, August 25, 2025
The World's Largest Radio Telescope -- It is in the Netherlands
Wednesday, July 23, 2025
The Red-Shifted Neutral Hydrogen Signal from the Cosmic Dark Ages is in the Range of our Direct Conversion Receiver
On the flight to the Dominican Republic I was listening to Fraser Cain's interview with Dr. Christiaan Brinkerink. I was kind of blown away when they started talking about where the neutral Hydrogen signal would be NOW, after the all of the cosmological red shift. Asked this question, Christiaan kind of casually responds that it would be "just above 7 MHz." He talks about this at 41 minutes and 41 seconds in the video above. He points out that this represents a redshift of about 200. Wow, that is just where our SolderSmoke Direct Conversion receivers tune, and where their PTO/VFOs operate. And we thought Radio Marti was a factor to consider! No wonder Christiaan and his colleagues want to go to the far-side of the moon. They want to get above the ionosphere, but they also want to get the shielding provided by the moon to protect them, I suppose, from signals like those being produced by the 40 meter ham band, and, (to a lesser extent) by devices like our little oscillator.
You can watch Fraser's interview with Christiaan above. It is really interesting and inspirational. Christiaan talks about dipole arrays, RFI, interferometers, sensitivity, signals of "several kHz" in width, dynamic range, and other topics known to us. Christiaan is an "Instrument Systems Engineer" at Radboud University. I think he deserves a ham radio license. Maybe he should build a SolderSmoke Direct Conversion receiver. Fraser should build one too.
Here are a couple of links to articles about this:
https://pmc.ncbi.nlm.nih.gov/articles/PMC10961189/
Thank you Fraser and Christiaan.
Tuesday, June 17, 2025
Sunday, June 8, 2025
Phil W1PJE, Director of MIT's Haystack Observatory, visits SolderSmoke East, Talks Radio with N2CQR and KK4DAS
Saturday, May 17, 2025
MIT's Haystack Observatory and Dr. Herb Weiss
He spent the bulk of his career developing radar when there was none in the United States. He joined the Radiation Lab at MIT, which was just being established to support the war effort during World War II, designing radars for ships and aircraft. In 1942, when England was in the throes of its air war with the Nazis, Herb went to England and installed radar in planes with a novel navigation system that he and a team had designed for the Royal Air Force. He later spent three years at the Los Alamos, New Mexico, laboratory improving instruments for the A-bomb. After seeing the need for a continental defense network against the Soviet missile threat, he returned to MIT to build it. If not for Herb, there also likely would be no MIT Haystack Observatory, a pioneering radio science and research facility."
Okay. I was born in New Jersey, and my first acquaintance with electronics was about the age of 12 or 13. We had a battery-operated radio, which didn't work, and I asked around about what do we do about it. They referred me to a man two blocks away, who was a radio ham it turned out. So I carried this monster with the big horn and, I guess, the dog sitting on the speaker to his house. We went down in the basement, and I was just fascinated. I was hooked right then and there. A year later I became a radio ham at the age of 13, 14 and literally have been in the field ever since, until I retired. I was fortunate enough to go to MIT as an undergraduate, and most of the people I ran into of that vintage didn't really have a hands-on feeling for electronics. By the time I got to MIT, I had built all kinds of things, including a TV set. Then it turned out that NBC was just trying to get their TV set on the air in New York on top of the Empire State Building."
Phil Erickson
Friday, April 19, 2024
Deep Space Station 43 -- Canberra, Australia
DSS-43 boasts a pointing accuracy of 0.005 degrees (18 arc seconds)—which is important for ensuring that it is pointed directly at the receiver on a distant spacecraft. Voyager 2 broadcasts using a 23-watt radio. But by the time the signals traverse the multibillion-kilometer distance from the heliopause to Earth, their power has faded to a level 20 billion times weaker than what is needed to run a digital watch. Capturing every bit of the incident signals is crucial to gathering useful information from the transmissions.
The antenna has a transmitter capable of 400 kilowatts, with a beam width of 0.0038 degrees. Without the 1987 upgrade, signals sent from DSS-43 to a spacecraft venturing outside the solar system likely never would reach their target.
Thursday, January 25, 2024
RIP Arno Penzias -- Co-discoverer of the Big Bang Cosmic Background Radiaton
Wednesday, September 20, 2023
The Art of Electronics #5 Paul Horowitz on SETI (and lots of other radio stuff)
Tuesday, December 13, 2022
Save the Antenna!
Monday, April 18, 2022
Ruby Payne-Scott and Early Australian Radio Astronomy
Wednesday, January 12, 2022
Looking at the Galaxy's Spiral Arms with a Dongle, a Raspberry Pi,and a Homebrew Antenna
Tuesday, October 26, 2021
SETI, Proxima Centauri, The Parkes Dish, and Intermodulation Distortion?
A cosmically interesting troubleshoot. But I'm not sure about their explanation. Why would the intermod disappear when they moved the Parkes Radio Telescope off of Proxima Centauri?



