Lesson 3: Radio Wave Propagation
Propagation at this level adds the specialized modes: Earth-Moon-Earth, meteor scatter, transequatorial and long path.
What you will learn
- E3A Electromagnetic Waves and Specialized Propagation: Earth-Moon-Earth (EME) communications; meteor scatter; microwave tropospheric and scatter propagation; auroral propagation; daily variation of ionospheric propagation; circular polarization
- E3B Transequatorial propagation; long-path propagation; ordinary and extraordinary waves; chordal hop; sporadic-E mechanisms; ground-wave propagation
- E3C Propagation prediction and reporting: radio horizon; effects of space-weather phenomena
1. Read
- How radio signals travel: VHF and UHF beyond the horizonHelps with E3A, E3B
- How radio signals travel: Ground waveHelps with E3B
- How radio signals travel: Line of sight and the radio horizonHelps with E3C
- How radio signals travel: When the Sun misbehavesHelps with E3C
- How radio signals travel: Checking conditions right nowHelps with E3C
- All 39 E3 questions with their answers and explanationsEvery group, with the rule or source behind each answer
2. Explore
- Propagation conditions
Move the time across a full day and watch the boundary between day and night sweep around the map.
- Grid square locator
Find the long path heading to a distant station: 180 degrees from the short path. Long path is most frequent on 40 and 20 meters.
This is exam question E3B06.
3. Practice
Practice one group at a time. A group is ready when you have answered every one of its questions and learned at least 80 percent of them; a question counts as learned when your last three answers to it were correct. To review quickly, go through this lesson’s questions as flashcards.
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