10 Meters

28.000 – 29.700 MHz

28 MHz is high enough that the ionosphere can only just bend it back down. It takes a hard-ionised F2 layer to do it, and that takes solar flux. Below about 90 the signal punches straight through into space and is simply gone.

WHY THE SUN HAS TO BE STRONG

28 MHz is high enough that the ionosphere can only just bend it back down. It takes a hard-ionised F2 layer to do it, and that takes solar flux. Below about 90 the signal punches straight through into space and is simply gone.

For example, at a flux of 115 the band opens, but thinly, and only while the sun is high. It shuts almost the moment the sun sets.

The exception is sporadic E in June and July — dense patches form in a lower layer and 10 meters goes wild for an hour with no warning, flux or no flux.

WHEN IT WORKS

BEST · Late morning to late afternoonWORST · After dark — almost alwaysWATCH · Sporadic E, May–Aug

WHO MAY TRANSMIT WHERE · 47 CFR §97.301

FREQUENCY (MHz)MODELICENSE CLASS
28.000–28.300CW / RTTY / dataTechnician and above, General, Advanced, Extra
28.300–28.500Voice — Novice & TechnicianTechnician and above, General, Advanced, Extra
28.500–29.000VoiceGeneral, Advanced, Extra
29.000–29.520Voice / AMGeneral, Advanced, Extra
29.520–29.600Satellite downlinkGeneral, Advanced, Extra
29.600–29.700FMGeneral, Advanced, Extra
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