Lesson 3: Radio Wave Propagation
Propagation explains when and where the HF bands open, which shapes everything you do on HF.
What you will learn
- G3A Sunspots and solar radiation; geomagnetic field and stability indices
- G3B Maximum Usable Frequency; Lowest Usable Frequency; short path and long path propagation; determining propagation conditions; ionospheric refraction
- G3C Ionospheric regions; critical angle and frequency; HF scatter; near vertical incidence skywave (NVIS)
1. Read
- How radio signals travel: The Sun drives HFHelps with G3A
- How radio signals travel: When the Sun misbehavesHelps with G3A
- How radio signals travel: Skip, the skip zone and the MUFHelps with G3B, G3C
- How radio signals travel: Checking conditions right nowHelps with G3B
- How radio signals travel: The ionosphereHelps with G3C
- How radio signals travel: Day and night by bandHelps with G3C
- All 37 G3 questions with their answers and explanationsEvery group, with the rule or source behind each answer
2. Explore
- Propagation conditions
Check today's planetary K index and 10.7 cm solar flux, then read what each one means for HF.
- Grid square locator
Find the short path and long path headings to a distant grid square. The long path points the opposite way, 180 degrees from the short path.
This is exam question G2D06.
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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