Practical_Antenna_Handbook_0071639586
C h a p t e r 2 : r a d i o - W a v e P r o p a g a t i o n 79 their ability to work DX find that a handful of profiles, one in the direction of each major population area, is sufficient. For example, a DXer or contest operator in the northeastern United States would profit most from profiles for 45 degrees (Europe, the Near East, and central Asia), 100 degrees (Africa), 170 degrees (Central and South America), 270 degrees (Australia and New Zealand), and 345 degrees (Western Australia, Japan, and the Far East). For this amateur, the 270-degree profile would also serve to identify terrain issues for most domestic U.S. beam headings, but amateurs in other parts of the country might need a sixth profile for that. Of course, the greatest and best use of HFTA profiles is before buying a site intended to be a stellar radio location! But it also has great utility after the fact for identifying how high one’s antennas for any given band must be to optimize the probabilities associated with the statistical nature of long-distance ionospheric propagation. The Magic of Radio Because so many of the known modes of propagation depend on external factors that are constantly varying over time, our ability to communicate—especially via the ionosphere—is a statistical one. Just because we were able to pick up the microphone and talk with another hobbyist halfway around the world on 20 m yesterday doesn’t mean we’ll be able to do it again today. The work we do to improve our antennas, the reading we do to understand the subtleties of propagation, the time we spend tuning across the bands, analyzing the noises we hear, listening for the weakest of signals—all are intended to tilt the odds more toward our favor. But ultimately we are at the mercy of Mother Nature, who is not above throwing us a curveball every now and then. Yet, for many of us, it is this statistical uncertainty that is at the very heart of the joy we find in communication by radio. For many, it is the unique sound of a weak signal fading in and out of the band noise that is the magic of radio. And, as in poker or bridge, where the number of different hands that can be dealt far exceeds the number that can be played in one’s lifetime, so too is there a nearly infinite variety of possible band conditions awaiting us each time we sit down at our receiver and put on the headphones. The unpredictability of ionospheric HF propagation is without a doubt one of the lifelong draws of radio communications for tens of thousands, the author included. It’s magic!
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C h a p t e r 2 : r a d i o - W a v e P r o p a g a t i o n 79<br />
their ability to work DX find that a handful of profiles, one in the direction of each major<br />
population area, is sufficient. For example, a DXer or contest operator in the northeastern<br />
United States would profit most from profiles for 45 degrees (Europe, the Near East,<br />
and central Asia), 100 degrees (Africa), 170 degrees (Central and South America), 270<br />
degrees (Australia and New Zealand), and 345 degrees (Western Australia, Japan, and<br />
the Far East). For this amateur, the 270-degree profile would also serve to identify terrain<br />
issues for most domestic U.S. beam headings, but amateurs in other parts of the<br />
country might need a sixth profile for that.<br />
Of course, the greatest and best use of HFTA profiles is before buying a site intended<br />
to be a stellar radio location! But it also has great utility after the fact for identifying how<br />
high one’s antennas for any given band must be to optimize the probabilities associated<br />
with the statistical nature of long-distance ionospheric propagation.<br />
The Magic of Radio<br />
Because so many of the known modes of propagation depend on external factors that<br />
are constantly varying over time, our ability to communicate—especially via the ionosphere—is<br />
a statistical one. Just because we were able to pick up the microphone and<br />
talk with another hobbyist halfway around the world on 20 m yesterday doesn’t mean<br />
we’ll be able to do it again today. The work we do to improve our antennas, the reading<br />
we do to understand the subtleties of propagation, the time we spend tuning across the<br />
bands, analyzing the noises we hear, listening for the weakest of signals—all are intended<br />
to tilt the odds more toward our favor. But ultimately we are at the mercy of<br />
Mother Nature, who is not above throwing us a curveball every now and then.<br />
Yet, for many of us, it is this statistical uncertainty that is at the very heart of the joy<br />
we find in communication by radio. For many, it is the unique sound of a weak signal<br />
fading in and out of the band noise that is the magic of radio. And, as in poker or bridge,<br />
where the number of different hands that can be dealt far exceeds the number that can<br />
be played in one’s lifetime, so too is there a nearly infinite variety of possible band conditions<br />
awaiting us each time we sit down at our receiver and put on the headphones.<br />
The unpredictability of ionospheric HF propagation is without a doubt one of the lifelong<br />
draws of radio communications for tens of thousands, the author included. It’s<br />
magic!