WEBVTT

NOTE MUF, LUF, and Choosing a Path

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<v Narrator>Two frequencies that bracket every path. For any two points on Earth at any moment, there is a window of usable frequencies with a ceiling and a floor.

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<v Pool>Question. What does MUF stand for?

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<v Pool>Answer. The Maximum Usable Frequency for communications between two points.

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<v Pool>Question. What does LUF stand for?

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<v Pool>Answer. The Lowest Usable Frequency for communications between two specific points.

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<v Narrator>Above the MUF, the ionosphere no longer bends the wave back, it passes through into space. Below the LUF, absorption is so heavy the signal does not survive the trip.

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<v Pool>Question. How does the ionosphere affect radio waves with frequencies below the MUF and above the LUF?

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<v Pool>Answer. They are refracted back to Earth.

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<v Pool>Question. What usually happens to radio waves with frequencies below the LUF?

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<v Pool>Answer. They are attenuated before reaching the destination.

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<v Narrator>Note the asymmetry in the failure modes: above the MUF your signal leaves; below the LUF it is absorbed. Two different physical mechanisms, both resulting in silence. Where in the window to operate.

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<v Pool>Question. Which frequency will have the least attenuation for long-distance skip propagation?

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<v Pool>Answer. Just below the MUF.

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<v Narrator>The highest frequency that still comes back. Higher frequencies penetrate deeper into the ionosphere before refracting, spending less time in the absorbing lower regions, so the closer to the MUF, the less loss.

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<v Narrator>The practical instruction is simple: work the highest band that is open. If you can hear the path on 15 metres, use 15 rather than 20. When the window closes.

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<v Pool>Question. What happens to HF propagation when the LUF exceeds the MUF?

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<v Pool>Answer. Propagation via ordinary skywave communications is not possible over that path.

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<v Narrator>The floor rises above the ceiling and there is no usable frequency at all. This happens during severe ionospheric disturbances, and it is why a path can be completely dead rather than merely difficult.

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<v Narrator>MUF depends on, the pool answers "all these choices are correct", the type of ionospheric layer involved, the amount of solar radiation, and the distance between stations.

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<v Narrator>Distance matters because a longer hop strikes the ionosphere at a shallower angle, and a shallower angle refracts a higher frequency. Hop distances.

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<v Narrator>Two numbers to memorise, and they follow directly from the height of the region:

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<v Pool>Question. What is the approximate maximum distance along the Earth's surface normally covered in one hop using the F2 region?

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<v Pool>Answer. 2,500 miles.

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<v Pool>Question. What is the approximate maximum distance along the Earth's surface normally covered in one hop using the E region?

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<v Pool>Answer. 1,200 miles.

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<v Narrator>F2 is roughly twice as high, so its hop is roughly twice as long. Geometry, not physics.

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<v Narrator>Useful consequence: a 5,000-mile contact is two F2 hops, and each hop costs absorption at both ionospheric passes and at the ground reflection between them.

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<v Narrator>Long paths are lossy in a way the numbers do not immediately suggest. Long path and short path. A radio wave can reach any point by the direct great-circle route or by going the other way round the world.

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<v Pool>Question. What is a characteristic of skywave signals arriving at your location by both short-path and long-path propagation?

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<v Pool>Answer. A slightly delayed echo might be heard.

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<v Narrator>The long path is longer, so it arrives later, tens of milliseconds, enough to hear as a distinct echo on your own or the other station's signal. It is unmistakable once you have heard it.

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<v Narrator>Long path is worth trying when short path is dead, particularly around sunrise and sunset, because the long way round may lie entirely in darkness or entirely in daylight when the short way does not.

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<v Narrator>Checking a band without transmitting.

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<v Pool>Question. Which of the following is a way to determine current propagation on a desired band from your station?

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<v Pool>Answer. Use a network of automated receiving stations on the internet to see where your transmissions are being received.

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<v Narrator>Reverse beacon networks and WSPR: automated receivers worldwide continuously report what they hear and how strongly.

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<v Narrator>Send a short CW call or a WSPR transmission and within a minute you can see, on a map, exactly where your signal landed.

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<v Narrator>This is a far better answer to "is the band open" than tuning around, and it is the modern replacement for guesswork. Seasonal and daily character.

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<v Pool>Question. Which of the following is typical of the lower HF frequencies during the summer?

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<v Pool>Answer. High levels of atmospheric noise or static.

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<v Narrator>Thunderstorms radiate broadband noise that propagates on the low bands. Summer nights on 80 and 160 metres are noisy for exactly the reason that summer afternoons have storms, often thousands of miles away.

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<v Narrator>Which is why the low bands are winter bands and the high bands are summer-and- solar-maximum bands. Check yourself. You can hear a station in Japan on both 20 and 15 metres. Which should you use, and why?

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<v Narrator>You hear an echo on your own signal. What is happening? A contact 4,000 miles away via F2. How many hops, minimum?

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<v Narrator>15 metres, the highest open band is closest to the MUF and suffers the least attenuation. Your signal is arriving by both short path and long path, and the long path's extra travel time is audible as a delayed echo. Two.

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<v Narrator>A single F2 hop covers about 2,500 miles.
