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Ted Shapas. K9 YOb'<br />

14925 Evers Avenue<br />

Dolton. Illinois 604J 9<br />

o a Better Angle<br />

Observations <strong>and</strong> Suggestions Involving IIF Radiation<br />

A ngle Manipulation<br />

When HF DX-getting tactics are discussed,<br />

sooner or later the subject will center<br />

around antennas, for the antenna, coupled<br />

with its geographic positioning. will ultimately<br />

make or break a DXer. A status is<br />

eventually achieved, however, when the<br />

serious DXer bas put up the largest <strong>and</strong><br />

tallest antenna he cared or dared to, or a<br />

point of "signal strength stagnation" is<br />

reached. For most of us this is a frustrating<br />

level. for it probably still means an S-unit or<br />

three gap between us <strong>and</strong> the big guns. Even<br />

if you feel you're near the top, however,<br />

there were undoubtedly times when these<br />

extra db would have come in h<strong>and</strong>y. This<br />

article is no magic panacea for combatting a<br />

W3CRA or WSVA in t he pileups, but<br />

knowing a little about radiation angle manipulation<br />

may give you something to think<br />

about along those lines.<br />

Low angle advantages<br />

I think many of us have operated enough<br />

to realize the importance placed upon an<br />

antenna with a very long boom perched<br />

upo n a very high tower. The fellows with the<br />

biggest combinations of these two, possibly<br />

coupled with an elegant location, constitute<br />

the big guns, or the big DXers <strong>and</strong> contest<br />

Winners.<br />

A maj or reason for their seeming invulnerability<br />

is the very low vertical rad iation<br />

angles associated with such an antenna combination.<br />

For normal F2 propagation paths,<br />

t he best sit uatio n is for your signal to reach<br />

a distant point in the least number of<br />

"hops" o r reflect ions. Up to about 2500<br />

miles or so , o ne hop propagation is po ssible,<br />

but after that, an earth reflection is neces-<br />

78<br />

sary. Now the signal is being decreased by a<br />

number of losses; most pertinent here are<br />

distance losses due to spacial. spreading, <strong>and</strong><br />

ground losses at each earthly hop. Distance<br />

loss is of course a function of distance; a<br />

lower reflection angle means less distance<br />

travelled <strong>and</strong> therefore less loss than a higher<br />

angle, although the difference may only<br />

amount to a db or two. Much more important<br />

are the ground lo sses. While sea reflections<br />

are less critical of incident angle,<br />

ground reflections may result in four or five<br />

db differences per hop between low <strong>and</strong> high<br />

angles, depending upon frequency (I). Here<br />

is one place where the big guns clean up!<br />

One or two less of these lossy earth hops<br />

experienced by signals approaching from a<br />

high angle <strong>and</strong> we're ta lking about S-units of<br />

difference. Fortunately, all is not this rosy<br />

for the people with the low take-off angl es,<br />

NBS observations - good news?<br />

The good news is that in most cases. these<br />

things I just talked about occu r only for<br />

"storybook" propagation unde r ideal conditions.<br />

What about the real world? W. F.<br />

Utlaut presented an interesting report along<br />

those lines in our National Bureau of St<strong>and</strong>ards<br />

research journal Radio Propagation<br />

where he made a detailed study o f radiation<br />

angle importance. The results were slightly<br />

astounding (2).<br />

Using a VOA transmitter in Munich,<br />

Germany , <strong>and</strong> receiving antennas in Boulder,<br />

Colorado (a receiver was also located in<br />

Slough, Engl<strong>and</strong> , but results were consistent<br />

with those in Boulder), all with carefully<br />

calculated radiation patterns, Utlaut attempter'<br />

to find out if low angles were that<br />

73 MAGA ZINE

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