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Solid State Shortwave Receivers For Beginners - The Listeners Guide

Solid State Shortwave Receivers For Beginners - The Listeners Guide

Solid State Shortwave Receivers For Beginners - The Listeners Guide

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High frequency signals pass straight through the E layer usually,<br />

and go on to the F2 layer where they are reflected back to earth. <strong>The</strong><br />

F2 layer is at a height of about 200 miles as compared to about 70<br />

miles for the E layer. This greater height of the F2 layer causes the<br />

reflected high frequency radio waves to be reflected back to the<br />

earth’s surface at a great distance from the transmitter, and it is<br />

partially this factor that makes the H.F. bands (10, 15 and 20 Metres)<br />

so good for DX reception. This type of propagation is represented by<br />

line A - E - F in the diagram.<br />

Another factor for the good DX reception on the H.F. bands is<br />

the absorbtion of the ground wave which prevents local transmitters<br />

from blotting out DX signsis. When listening on the 20 Metres amateur<br />

band it is quite common to hear a relatively local station in contact with<br />

one several thousands of miles away. Often the distant station provides<br />

a really strong signal whereas the local one is barely perceptible. In fact,<br />

when listening on the 20 Metre band only very rarely will a British<br />

station be heard at all.<br />

In order for a signal to pass from one side of the earth to the<br />

other it has to bounce from the atmosphere to the earth, back up to<br />

the atmosphere and then down to earth again for several cycles in order<br />

for it to negotiate the curvature of the earth’s surface.<br />

How well, or otherwise, the signals are reflected by the F2 layer<br />

is largely dependent upon unpredictable events, and the sun is a major<br />

factor here as it is it’s radiation that ionises the relevant layer of the<br />

atmosphere. It is quite possible for an H.F. band to suddenly have a<br />

proliferation of DX signals which disappear a few hours later just as fast<br />

as they arrived. <strong>For</strong> quite long periods the H.F. bands can seem to be<br />

completely dead, particularly towards the upper end of the S.W.<br />

frequency spectrum. <strong>The</strong>refore one should not be too perturbed if<br />

a newly constructed receiver does not seem to operate as well on the<br />

H.F. bands as it does on the L.F., ones. This is probably due to a lull<br />

in the propagation conditions on the H.F. bands rather than because<br />

of some fault in the receiver.<br />

Broadcast Bands<br />

<strong>The</strong>re are twelve broadcast bands and their frequency limits are<br />

shown in the table below. Note however, that broadcast stations tend<br />

to sprawl outside these limits, and they are not adhered to as strictly as<br />

in the case of the amateur bands.<br />

120 Metres 2.3 to 2.495 MHZ<br />

90 Metres 3.2 to 3.4 MHZ<br />

75 Metres 3.9 to 4.0 MHZ<br />

60 Metres 4.75 to 5.06 MHZ<br />

49 Metres 5.95 to 6.2 MHZ<br />

10

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