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Solar
SFI 128
SN 113
A 18
K 2 Quiet
X-Ray C1.2
Wind 554.7 km/s
Aurora 3
Updated 22:30 UTC HamQSL · N0NBH
Day 80/40m Fair 30/20m Good 17/15m Good 12/10m Fair
Night 80/40m Good 30/20m Good 17/15m Good 12/10m Poor

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E3: Radio Wave Propagation

Subelement E3 covers advanced radio wave propagation — the physical mechanisms that determine how and where amateur radio signals travel. This subelement addresses three groups: electromagnetic wave fundamentals and specialized propagation modes (EME, meteor scatter, tropospheric ducting, aurora, and circular polarization); advanced ionospheric propagation including transequatorial propagation, long-path, chordal hop, sporadic-E, and ground wave; and space weather effects on propagation including solar indices, the interplanetary magnetic field, and propagation prediction tools.

The Extra exam draws three questions from E3. Each group contributes one question. Mastering the specific conditions, distances, frequencies, and physical causes for each propagation mode is essential.

Key point: E3 requires precise knowledge — not general familiarity. Know the exact distance ranges, time-of-day conditions, frequency bands, geomagnetic indices, and solar parameters that define each propagation mode and space-weather phenomenon.

Study These Topics

E3A: Specialized Propagation

EME geometry and libration fading, electromagnetic wave structure, meteor scatter in the E region, tropospheric ducting over water, auroral propagation and CW, MUF and darkness, circular polarization.

Study E3A

E3B: Advanced Propagation Modes

Transequatorial propagation (TEP) distance and timing, long-path on 40m/20m, ordinary and extraordinary waves, chordal-hop mechanics, sporadic-E at solstices, ground-wave polarization and frequency effects.

Study E3B

E3C: Propagation Prediction and Space Weather

Solar flares and blackouts, A-index and K-index, Bz orientation, auroral oval absorption, VHF/UHF radio horizon, solar flare classes, geomagnetic storm scales, VOACAP, 304A solar parameter.

Study E3C
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