The explanations for all ten questions sit on this sheet. Pick an answer on the left and the matching card lights up.
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G3B01 Explanation 1
Key D — The steepest angle of radiation that is still returned to earth
Steeper than the critical angle and the wave penetrates the layer and is lost to space. This is why NVIS on 40 metres works only up to a point: there is a maximum angle that the F layer can turn back on that frequency.
Rule Fundamentals - critical angle
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G3B02 Explanation 2
Key C — About 4,000 kilometres
A good single hop on the F2 layer reaches roughly 4,000 kilometres, so an intercontinental contact of 12,000 kilometres is three hops. Each hop adds loss and each requires the geometry to work out, which is why multi-hop paths are harder than they look.
Rule Fundamentals - hop distance
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G3B03 Explanation 3
Key B — The signal travels the great-circle route in the opposite direction from the short path
Two stations are joined by two great-circle routes, and the long path is the one going the other way round the globe. It becomes the better route when the short path is in daylight or in heavy absorption, which is why long-path contacts cluster around sunrise and sunset.
Rule Fundamentals - long path
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G3B04 Explanation 4
Key A — Static from distant thunderstorms raises the noise level far above the signals
Atmospheric noise is strongest at the lowest frequencies, and summer thunderstorms across a continent make 160 metres a wall of static. The band improves markedly in winter, when the static quietens and the hours of darkness are long.
Rule Fundamentals - atmospheric noise
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G3B05 Explanation 5
Key D — Enhanced propagation across the geomagnetic equator between stations at similar magnetic latitudes
Transequatorial paths cross the magnetic equator and are often stronger than the distance suggests, an effect seen on 6 metres and 10 metres in particular. The geometry requires the two ends to sit at roughly mirror-image magnetic latitudes.
Rule Fundamentals - transequatorial propagation
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G3B06 Explanation 6
Key C — The level of ionisation, and therefore how often the higher HF bands are usable
During a solar maximum the F2 layer is dense and the MUF climbs, so 10 and 15 metres open to the world for years at a time. During a minimum those bands may be usable only sporadically, and 20 metres carries most of the long-haul traffic.
Rule Fundamentals - solar cycle
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G3B07 Explanation 7
Key B — Transmitting a one-way signal from a known location so operators can tell whether a band is open
Beacons transmit continuously on fixed frequencies, most famously across the 10 metre and 6 metre bands, so hearing one tells you the path from that region is open right now. Software such as WSPR extends the same idea by reporting reception automatically.
Rule 47 CFR §97.203 - beacon stations
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G3B08 Explanation 8
Key A — Sporadic E patches are small, drifting and short-lived
The E-region patches that refract 50 MHz are typically tens of kilometres across and drift with the wind, so a path opens and closes as the patch moves. Operators monitor beacons and spotting networks precisely because the window is so short.
Rule Fundamentals - sporadic E
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G3B09 Explanation 9
Key D — Ground wave follows the earth's curvature better at lower frequencies and is attenuated rapidly as frequency rises
Ground wave depends on the conductivity of the earth and the frequency: at 1.8 MHz it can cover a hundred kilometres or more over good soil, while at 144 MHz it is limited to little more than line of sight. This is why HF mobile stations keep in touch on 40 or 80 metres over the same distance where 2 metres fails.
Rule Fundamentals - ground wave
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G3B10 Explanation 10
Key D — The contact is being made by long path, with the signal travelling the other way around the world
A signal from the reciprocal bearing, deficient in high audio frequencies and often accompanied by an echo, is the signature of long-path propagation. It usually means the short path is in daylight or under absorption while the long path is in darkness.
Rule Fundamentals - long path signatures