WEBVTT NOTE Transequatorial, Long Path, and Chordal Hop 1 00:00:00.000 --> 00:00:03.360 Elevation angle decides hop length. 2 00:00:03.360 --> 00:00:14.186 Question. What effect does lowering a signal's transmitted elevation angle have on ionospheric HF skip propagation? 3 00:00:15.086 --> 00:00:20.366 Answer. The distance covered by each hop increases. 4 00:00:20.966 --> 00:00:27.778 Geometry: a shallower angle strikes the ionosphere further away and comes down further still. 5 00:00:27.778 --> 00:00:42.866 This is the mechanism behind everything the General antennas module said about antenna height, and it is why a DX antenna is judged by its takeoff angle rather than its gain figure. There is a diagram here. 6 00:00:42.866 --> 00:00:55.318 Four stacked bands above the Earth's surface. The D region sits from about 60 to 90 kilometres and absorbs signals below 10 megahertz during daylight, vanishing at night. 7 00:00:55.318 --> 00:01:09.747 The E region from about 90 to 150 kilometres refracts and supports sporadic E, weakening at night. The F1 region from about 150 to 250 kilometres exists in daytime only and merges into F2 at night. 8 00:01:09.747 --> 00:01:23.883 The F2 region from about 250 to 400 kilometres is the highest and supports the longest single-hop paths, persisting day and night. Every path in this lesson is a consequence of those altitudes. 9 00:01:23.883 --> 00:01:38.166 A refraction from F2 at 300 km reaches much further than one from E at 100 km, and a chordal hop stays inside the F region rather than descending between refractions. Transequatorial propagation. 10 00:01:38.166 --> 00:01:46.406 Question. Where is transequatorial propagation (TEP) most likely to occur? 11 00:01:47.306 --> 00:01:58.570 Answer. Between points separated by 2,000 miles to 3,000 miles over a path perpendicular to the geomagnetic equator. 12 00:01:59.170 --> 00:02:07.570 Question. What is the approximate maximum range for signals using transequatorial propagation? 13 00:02:08.470 --> 00:02:12.190 Answer. 5,000 miles. 14 00:02:12.790 --> 00:02:19.961 Question. At what time of day is transequatorial propagation most likely to occur? 15 00:02:20.861 --> 00:02:24.941 Answer. Afternoon or early evening. 16 00:02:25.541 --> 00:02:32.387 Roughly equal distances either side of the magnetic equator, in the late afternoon. 17 00:02:32.387 --> 00:02:49.791 TEP works at frequencies well above the ordinary MUF, it regularly opens 6 metres between the Americas and Europe when nothing else is moving, because the equatorial ionosphere is unusually dense and structured. 18 00:02:49.791 --> 00:02:50.781 Chordal hop. 19 00:02:50.781 --> 00:02:55.981 Question. What is chordal-hop propagation? 20 00:02:56.881 --> 00:03:05.785 Answer. Successive ionospheric refractions without an intermediate reflection from the ground. 21 00:03:06.385 --> 00:03:11.705 Question. What is the effect of chordal-hop propagation? 22 00:03:12.605 --> 00:03:21.448 Answer. The signal experiences less loss compared to multi-hop propagation, which uses Earth as a reflector. 23 00:03:22.048 --> 00:03:32.070 Ordinary multi-hop bounces off the ground between ionospheric refractions, and each ground reflection costs several decibels. 24 00:03:32.070 --> 00:03:42.572 Chordal hop skims along inside the ionosphere, refracting repeatedly without ever touching down, so the losses simply do not occur. 25 00:03:42.572 --> 00:03:52.674 This is why some very long paths are far stronger than a hop count would predict, and it is closely related to TEP. Long path. 26 00:03:52.674 --> 00:04:02.485 Question. Which of the following paths is most likely to support long-distance propagation on 160 meters? 27 00:04:03.385 --> 00:04:08.027 Answer. A path entirely in darkness. 28 00:04:08.627 --> 00:04:15.827 Question. On which of the following amateur bands is long-path propagation most frequent? 29 00:04:16.727 --> 00:04:20.607 Answer. 40 meters and 20 meters. 30 00:04:21.207 --> 00:04:37.542 A darkness path has no D-region absorption anywhere along it, so the low bands carry worldwide. The long way round is often entirely dark when the short way is not, which is exactly when long path opens. 31 00:04:37.542 --> 00:04:49.934 Forty and twenty are the bands where it is common: high enough to escape the worst absorption, low enough that the MUF supports the distance. Ground wave. 32 00:04:49.934 --> 00:04:56.214 Question. What type of polarization is supported by ground-wave propagation? 33 00:04:57.114 --> 00:04:59.754 Answer. Vertical. 34 00:05:00.354 --> 00:05:09.474 Question. How does the maximum range of ground-wave propagation change when the signal frequency is increased? 35 00:05:10.374 --> 00:05:13.190 Answer. It decreases. 36 00:05:13.790 --> 00:05:28.484 Ground wave follows the Earth's curvature by dragging along a conductive surface, which only works for a vertically polarised wave, a horizontal one is shorted out by the ground. 37 00:05:28.484 --> 00:05:42.270 And higher frequencies attenuate faster, which is why AM broadcast at 1 MHz has a useful ground wave and 28 MHz effectively does not. Ordinary and extraordinary waves. 38 00:05:42.270 --> 00:05:48.230 Question. What are "extraordinary" and "ordinary" waves? 39 00:05:49.130 --> 00:05:57.410 Answer. Independently propagating, elliptically polarized waves created in the ionosphere. 40 00:05:58.010 --> 00:06:16.459 The Earth's magnetic field makes the ionosphere birefringent: a single incoming wave splits into two components that propagate independently, with different velocities, different absorption, and opposite senses of elliptical polarisation. 41 00:06:16.459 --> 00:06:32.815 They arrive at slightly different times and combine unpredictably, which is a large part of why HF signals fade the way they do, and why the General track's answer that "either polarisation works on HF" is true. 42 00:06:32.815 --> 00:06:38.164 Whatever you transmit, the ionosphere re-sorts it. Sporadic E, timed. 43 00:06:38.164 --> 00:06:45.169 Question. At what time of year is sporadic-E propagation most likely to occur? 44 00:06:46.069 --> 00:06:51.829 Answer. Around the solstices, especially the summer solstice. 45 00:06:52.429 --> 00:06:59.429 Question. At what time of day is sporadic-E propagation most likely to occur? 46 00:07:00.329 --> 00:07:04.447 Answer. Between sunrise and sunset. 47 00:07:05.047 --> 00:07:23.581 Summer, daytime, with a well-known secondary peak around the winter solstice. The Technician track said "usually early summer"; this is the precise version, and it tells a 6 metre operator when to be listening. 48 00:07:23.581 --> 00:07:42.998 Check yourself. Why is chordal-hop propagation stronger than multi-hop over the same distance? It is 3 pm and you are 2,500 miles north of the magnetic equator, hoping to work someone 2,500 miles south of it on 6 metres. 49 00:07:42.998 --> 00:07:49.264 What mode of propagation? Why does ground wave need a vertical antenna? 50 00:07:55.264 --> 00:08:04.768 It refracts within the ionosphere without ground reflections, and each ground reflection in multi-hop costs several decibels. 51 00:08:04.768 --> 00:08:11.992 Transequatorial propagation, the right geometry, the right distance, and the right time of day. 52 00:08:11.992 --> 00:08:23.397 Ground wave propagates by following a conductive surface, which only works for a vertically polarised wave; a horizontal one is shorted by the ground.