At 522,000,000 miles per watt, Voyager could be the ultimate in QRP ... if you have the right antenna.
For most HAMs the experience of seeing sub-one watt WSPR signals decoded from across the globe is enough of a thrill. However, the fine folks at the National Radio Astronomy Observatory have taken this a little further and used the Very Long Baseline Array radio telescope to precisely pinpoint the position of the Voyager 1 space probe.
While the layperson might see detecting the glimmer of 22 watts across the vastness of space miraculous, the amateur radio community can see this feat as the natural evolution and refinement of the technology and medium we know and love.
Earlier this year, the National Science Foundation's Very Long Baseline Array telescope turned its gaze to NASA's famed Voyager 1 and captured an image of this iconic spacecraft's faint radio signal. The Green Bank Telescope also detected Voyager's signal, picking it out from the background radio noise in less than one second.
Astronomers using the National Science Foundation's (NSF) Very Long Baseline Array (VLBA) and Green Bank Telescope (GBT) spotted the faint radio glow from NASA's famed Voyager 1 spacecraft -- the most distant man-made object.
According to NASA's Jet Propulsion Laboratory (JPL), the VLBA imaged the signal from Voyager 1's main transmitter after the spacecraft had already passed beyond the edge of the heliosphere, the bubble of charged particles from the Sun that surrounds our Solar System.
Using NASA's Deep Space Network, JPL continually tracks Voyager and calculates its position on the sky, which is known as the ephemeris. Since the VLBA has the highest resolution, or ability to see fine detail, of any full-time astronomical instrument, NRAO astronomers believed they could locate Voyager's ephemeris position with unprecedented precision. This is unrelated to Voyager's distance from the Sun or position relative to the heliosphere.
The initial observations, which were made on February 21, placed Voyager very near, but not precisely at its predicted location. The difference was a few tenths of an arcsecond. An arcsecond is the apparent size of a penny as seen from 2.5 miles (4 kilometers) away. The second observations on June 1 produced similar results.
"It is possible that these observations are at the milliarcsecond [one-thousandth of an arcsecond] level, or better," said NRAO scientist Walter Brisken, who led the observations with the VLBA. At 11.5 billion miles -- Voyager's approximate distance at the time of the initial observations -- one milliarcsecond would be roughly 50 miles across.
Voyager's main transmitter shines at a feeble 22 watts, which is comparable to a car-mounted police radio or -- in visible light -- a refrigerator light bulb. Though incredibly weak by the standards of modern wireless communications, Voyager's signal is astoundingly bright when compared to most natural objects studied by radio telescopes.
"The ability to pinpoint the location of Voyager and other spacecraft is critical as we explore the inner Solar System and beyond," said Brisken. "The NRAO's VLBA has the capability to do this vital task with unprecedented precision."
Voyager 1, which was launched in 1977, is now headed away from the Sun at a speed of about 38,000 miles per hour.
In a remarkably sensitive complementary observation, the NRAO's Green Bank Telescope (GBT), which is the world's largest fully steerable radio telescope, easily detected Voyager's signal, picking it out from the background radio noise in less than one second.
"Voyager is the first man-made object to penetrate the interstellar medium, and we really want to be able to receive the data from this new frontier," said NRAO scientist Toney Minter, who oversaw the Green Bank observations. "This information will provide many clues about how the interstellar medium behaves and how the Sun interacts with it."
"NRAO's instruments have the capability to provide the most accurate position information of distant spacecraft like Voyager," said NRAO Director Tony Beasley. "The remarkable sensitivity of GBT and VLBA's sharp vision are essential for discovery but also have unique capabilities that have enabled us to make this contact with one of humanity's most ambitious missions of exploration."
The VLBA is a system of radio antennas located across the United States from Hawaii to St. Croix. The antennas work together as a single telescope nearly 5,000 miles across, giving the VLBA its ability to see fine details. Only seven of the VLBA's full complement of 10 antennas were used to make these observations.
The 100-meter GBT is located in the National Radio Quiet Zone and the West Virginia Radio Astronomy Zone, which protect the incredibly sensitive telescope from unwanted radio interference. The GBT observations were made by NRAO scientists Toney Minter and Frank Ghigo, and Green Bank Director Karen O'Neil.
According to a resent paper published in the American Institute of Physics, nanoscale vacuum "tubes" manufactured using conventional chip making techniques have operated at frequencies as high as .46 THz..jpg){kind=spacer}
The increased operating frequency comes about because of the speed at which electrons travel through different materials. The speed of electron travel through silicon is comparatively slow, through graphine it is approximately 100 times faster and through a vacuum it approaches the speed of light.
If you have looked through my blog you'll know that I have a soft spot for tubes and tube technology. At a time when our understanding of electron mechanics and quantum theory was still in development the manufacture of advanced vacuum tubes was part science, part physics and part art.
Special purpose tubes were developed in their thousands to meet the needs of commercial, scientific and industrial applications. Their form and functions were as varied as the devices they were installed in. Sometimes tubes were developed to meet a specific need and sometimes new tubes were developed for applications not yet in existence.
The PDF file is available from Adafruit Industries or a copy is also here. Once you print it out, a little cutting and folding should produce something like the example of the right. The Adafruit design uses brass paper fasteners (remember those?) but any fastener could be used that would allow the wheel inside to rotate freely. It would be best to print on heavy card stock if you have the ability as it will give the calculator some strength.
