It's no secret that I'm a radio amateur (ham radio operator); I've talked
about that hundreds of times over the life of the blog. There has been a
Radio Sunday
series and a specific
Ham Radio Series. This will go with the ham radio series.
Something I haven't mentioned as often, but still have several times, is that
one of my hobbies as far back as I can recall has been astronomy and
telescopes. I haven't been active in that for a while, but there are posts
here about that I found by going back and searching the blog for specific
words. I've built telescopes, reflectors from grinding the mirror from a plate
of glass, and refractors from things like copier lenses. Some
background here, although not related to tonight's post.
As an amateur astronomer, I've gone to places near and far where I could
observe a meteor shower that was supposed to be particularly good. People who
aren't in to this hobby generally aren't aware that there are
regularly recurring meteor showers several times a year. If you follow meteor showers to observe the pretty light streaks the
meteors leave, you quickly learn that showers are best in the early morning
hours, or between midnight and first light. If the moon is close to full and
bright, it can wipe out the best of showers. The reason for the timing
is that as the Earth moves in its orbit, the rotation that brings night and
day rolls the planet onto some meteors, so more are seen. The meteors have to
be moving faster to catch up with the planet.
Back in the 1950s, hams discovered that the trail created in the upper
atmosphere by meteors burning up acted like a radio reflector, as if the
ionosphere was enhanced. The effect is most beneficial to VHF stations which
typically don't have regular, predictable ionospheric propagation. In the
early days, this was done with Morse code, or CW as the hams typically call it
(CW for Continuous Wave). Now that we're firmly in the age of computer
assisted modulation modes, most people trying to bounce signals off the meteor
trails are using a computer assisted mode. The most popular appears to be
MSK144
(.pdf alert).
MSK stands for minimum shift keying, a form of continuous-phase
frequency-shift keying (FSK) with shift equal to half the baud rate. MSK144
uses message frames of 144 bits and modulation at tone frequencies 1000 and
2000 Hz to transmit channel symbols at keying rate of 2000 baud. The
resulting audio waveform can be viewed as a form of offset quadrature
phase-shift keying (OQPSK) with individual pulses shaped like the first
half-period of a sine wave.
Although there are other modes still used for meteor scatter, this is the
dominant mode.
So how do you operate meteor scatter? Have contacts with people hundreds to
perhaps 1500 miles or more by bouncing a signal off a meteor trail?
This is why the talk of meteor showers. This time of year has an annual shower
named after the constellation it appears to radiate from, Lyra (the lyre) and
called the Lyrid shower. Meteor showers don't just happen, they ordinarily
happen when the Earth goes through the trail left by comet; the Lyrids are the
trail of comet called C/1861 G1 (Thatcher). That's right, it's a comet that
was first named in 1861, and it's a long period comet with around a 422-year
orbit. It's expected to return around 2283. Thatcher is the discoverer.
The Lyrids are predicted to peak Monday morning. Interestingly, another shower
is already starting to build, coming to its peak two weeks later on May 5th.
This is called the Eta Aquariids because it appears to radiate from close to
the star Eta Aquarii. This shower is dust from the trail of Halley's comet.
Halley's comet is another relatively long period comet although at 76 years
quite a bit shorter than Thatcher's; its last close approach to the sun or
perihelion was in 1986, and its next perihelion will be in 2061. I remember
taking my son to the beach to see Halley's comet; he was five. I haven't asked
him if he remembers that in years.
Given the shower to provide the meteors and the software to interface to your
radio to modulate and demodulate the data stream, if your antenna is
directional, it makes sense to point it toward the radiant because the trails
will be denser there. Most people use a 15 second transmit period followed by
15 seconds receive. The protocol is that if you're trying to contact people to
your east, you transmit on the minute and half minute marks - or 0 and 30
seconds. Those are referred to as the even intervals, so they give rise to the
acronym
PETE: Point East Transmit Even.
If you're trying to contact people to your west, you transmit on the 15 and
45 second marks.
You'll get the best reflections where the trails are the densest, so unlike
the case with other modes, you don't necessarily point your antenna at the
person your contacting. It works best if you're both pointed at the radiant.
Remember, the radiant is like everything else in the sky: it raises in the
East and sets in the West. The exact position in the sky of the radiant
isn't extremely important, but the astronomy observing-oriented websites help
you learn where the radiant is. There's a program aimed at ham use that seems
helpful,
called Virgo.
It's important to know that while the astronomy websites are concerned with
the peak number of meteors visible per hour, and the Lyrids aren't impressive
that way, the showers are perfectly usable for radio after first light and
well into the morning. The things that make a shower a highlight for visual
observation don't mean much to radio use. I've played at this mode only a few
times, and copied signals off the meteor trails until 9 to 10 AM.