WEBVTT

NOTE EME, Meteor Scatter, and Wave Properties

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<v Narrator>Wave properties, precisely. Three facts the Technician track stated loosely and Extra tests exactly.

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<v Pool>Question. How are the component fields of an electromagnetic wave oriented?

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<v Pool>Answer. They are at right angles.

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<v Pool>Question. In what direction does an electromagnetic wave travel?

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<v Pool>Answer. It travels at a right angle to the electric and magnetic fields.

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<v Narrator>All three, electric field, magnetic field, direction of travel, are mutually perpendicular.

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<v Pool>Question. What determines the speed of electromagnetic waves through a medium?

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<v Pool>Answer. The index of refraction.

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<v Narrator>Which is where velocity factor comes from: a coax's dielectric has an index of refraction, and the wave slows accordingly.

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<v Pool>Question. What are circularly polarized electromagnetic waves?

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<v Pool>Answer. Waves with rotating electric and magnetic fields.

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<v Narrator>The rotation produced by two perpendicular linear antennas fed in quadrature, from the antennas module. Earth-Moon-Earth.

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<v Pool>Question. What is the approximate maximum separation measured along the surface of the Earth between two stations communicating by EME?

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<v Pool>Answer. 12,000 miles, if the moon is "visible" by both stations.

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<v Narrator>The only requirement is that both stations can see the Moon at once, which, given the Earth's curvature, means up to about half the planet apart.

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<v Pool>Question. What characterizes libration fading of an EME signal?

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<v Pool>Answer. A fluttery, irregular fading.

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<v Narrator>The Moon wobbles slightly in its rotation (libration), so the many reflecting features on its surface shift relative to each other and their reflections combine and cancel irregularly.

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<v Narrator>It is multipath, on a 480,000-mile path, and it gives EME signals their characteristic flutter.

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<v Pool>Question. When scheduling EME contacts, which of these conditions will generally result in the least path loss?

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<v Pool>Answer. When the Moon is at perigee.

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<v Narrator>Perigee is the Moon's closest approach, around 356,000 km against 406,000 at apogee.

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<v Narrator>Path loss goes as the fourth power of distance for a two-way reflection, so the difference between perigee and apogee is a couple of decibels.

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<v Narrator>On a path with almost no margin, a couple of decibels is worth scheduling around. Meteor scatter.

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<v Pool>Question. When a meteor strikes the Earth's atmosphere, a linear ionized region is formed at what region of the ionosphere?

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<v Pool>Answer. The E region.

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<v Narrator>Around 100 km, the E region altitude, which is why meteor-scatter distances resemble sporadic-E distances.

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<v Pool>Question. Which of the following frequency ranges is most suited for meteor-scatter communications?

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<v Pool>Answer. 28 MHz - 148 MHz.

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<v Narrator>Ten metres through 2 metres, with 6 metres the sweet spot from the Technician track. Below that the ionosphere carries the signal anyway; above it the trails do not reflect well. Auroral propagation.

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<v Pool>Question. What is most likely to result in auroral propagation?

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<v Pool>Answer. Severe geomagnetic storms.

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<v Pool>Question. Which of these emission modes is best for auroral propagation?

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<v Pool>Answer. CW.

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<v Narrator>Auroral reflection Doppler-smears a signal badly, the "raspy" quality from the Technician track. SSB voice becomes unintelligible; CW survives because a smeared tone is still a tone with recognisable timing.

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<v Narrator>This is the general rule for degraded paths: the less structure the signal carries per second, the more abuse it survives. Tropospheric ducting.

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<v Pool>Question. Atmospheric ducts capable of propagating microwave signals often form over what geographic feature?

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<v Pool>Answer. Large bodies of water.

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<v Narrator>Water surfaces produce the stable temperature inversions ducting needs. This is why long microwave paths over sea are routine and the same paths over land are not.

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<v Pool>Question. What is a typical range for tropospheric duct propagation of microwave signals?

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<v Pool>Answer. 100 miles to 300 miles.

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<v Narrator>When the MUF drops.

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<v Pool>Question. What should be done to continue a long-distance contact when the MUF for that path decreases due to darkness?

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<v Pool>Answer. Switch to a lower frequency HF band.

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<v Narrator>Directly from the General MUF lesson: above the MUF the signal leaves. Move down until you are below it again, which is why an evening on HF is a walk down the bands as the ionosphere weakens. Check yourself.

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<v Narrator>Why does a perigee EME schedule matter when the difference is only about 2 dB? An aurora is running and you want to work it. Which mode, and why not SSB? The band goes quiet mid-contact. Up a band or down?

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<v Narrator>Because an EME path has almost no margin, two decibels is the difference between copy and no copy. CW. Auroral Doppler smearing destroys voice intelligibility, and a smeared tone is still readable. Down.

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<v Narrator>The MUF has fallen below your frequency; a lower band brings you back under it.
