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HF band characteristics: what each band does

One table that tells you which band to try, and why it is behaving that way.

The short answer

Forty metres is the most reliable HF band in the country and works day and night out to about 1,500 miles. Twenty metres is the main worldwide daytime band and works in every year of the solar cycle. Ten and fifteen metres are spectacular near solar maximum and largely closed near minimum.

Most reliable band
40 m
Main DX band
20 m
Best at solar max
10 m
Quietest band
17 m
Noisiest in summer
80 m
Magic band
6 m

Bands have personalities. Not in a poetic sense: each one behaves differently because of how the ionosphere treats its frequency, how large an antenna it needs, and what kind of operator has therefore gathered there. Knowing that in advance saves a great deal of tuning around.

This table is the summary. The physics behind it is in HF propagation basics, and where the modes live within each band is in the US amateur band plan.

The HF bands

Band by band

Range, timing and antenna size for every HF band

BandBest timeTypical rangeHalf waveCharacter
160 mWinter nightsRegional to worldwide246 ftA specialist band, big antennas, dedicated crowd
80 mNights, best in winter300 to 1,500 miles125 ftRegional nets, rag chews, noisy in summer
60 mNights and dawn200 to 800 miles87 ftFive channels, low power, emergency use
40 mEvening and night300 to 2,500 miles66 ftThe most reliable band, always active
30 mDay and night500 to 3,000 miles46 ftCW and data only, quiet and stable
20 mDaylight, all yearWorldwide33 ftThe main DX band, busiest in the afternoon
17 mDaylightWorldwide26 ftQuiet, relaxed, no contests permitted
15 mDaylight, good yearsWorldwide22 ftExcellent at solar maximum, dead at minimum
12 mDaylight, good yearsWorldwide19 ftUnderused, rewarding when open
10 mDaylight, and sporadic EWorldwide or local17 ftSpectacular at solar max, empty otherwise
6 mWarm months, sporadic E500 to 1,500 miles9 ftThe magic band, sudden dramatic openings
2 mAny time30 to 100 miles3 ft 2 inRepeaters, satellites, weak signal work
70 cmAny time20 to 60 miles1 ft 3 inRepeaters, digital voice, satellites

Range figures assume a typical station with a wire antenna at moderate height. A good antenna at height and open conditions produce much more; a compromise antenna in a noisy location much less. Half wave lengths are from the dipole length chart.

Choosing a band by what you want

Talking to people 100 to 300 miles away
Eighty metres at night, or 40 metres during the day with a low antenna that radiates at a high angle. This is the range where regional nets and emergency traffic live, and where a low dipole is the correct antenna rather than a compromise.
Worldwide contacts on a normal station
Twenty metres in the afternoon, every day of the solar cycle. Forty metres in the evening. Those two bands carry most of the worldwide contacts made by ordinary stations with wire antennas.
A quiet band for a long conversation
Seventeen metres. Contests are not permitted there, so it stays civil, and it is open worldwide in daylight in most conditions.
Something dramatic
Six metres in the warmer months. Sporadic E openings appear without warning and produce strong signals over 500 to 1,500 miles for minutes or hours. It is the reason the band is called magic.
Reliable local communication
Two metres through a repeater, at any time, in any conditions. It is the band that works when nothing else does because it does not depend on the ionosphere at all.
Working the world with a compromise antenna
Twenty metres on FT8. The band is open most days and the mode tolerates a signal 20 dB weaker than voice needs.

Noise by band

Noise

What limits reception on each band

BandDominant noiseSeasonal pattern
160 and 80 mAtmospheric static and household devicesMuch worse in summer thunderstorm season
40 mAtmospheric plus broadcast splatter at nightWorse in summer
30 and 20 mMan-made, switching supplies and LED driversConstant year round
17 to 10 mMan-made, and often very quietConstant, lowest of the HF bands
6 mMan-made and ignition noiseConstant
2 m and 70 cmLocal electrical and intermodulationWorst near commercial transmitters

The lower the band, the more the noise floor is set by nature and the less you can do about it. The higher the band, the more it is set by devices in your own house, which you can do a great deal about. See radio noise and RFI hunting.

Antennas for each band range

Matching the antenna to the band

The lower the band, the bigger the antenna and the more the compromises bite.

Icom IC-7300

Icom

Icom IC-7300

A spectrum scope that shows at a glance whether a band is open or simply empty.

Check price$1,255.74

Common questions

Questions people ask about this

Which HF band should a beginner start on?

Forty metres in the evening and twenty metres in the afternoon. Between them they carry most of the activity a normal station will find, they work in every year of the solar cycle, and both need an antenna a typical garden can support. Twenty metres in particular is reliable worldwide in daylight even when solar activity is low.

Why is 80 metres so noisy in summer?

Because atmospheric noise from distant thunderstorms is far stronger at low frequencies, and thunderstorm activity peaks in the warm months. That noise is natural and there is very little you can do about it beyond a directional receive antenna or a noise blanker. Eighty metres becomes a much better band in winter for exactly this reason.

What is the magic band and why is it called that?

Six metres, at 50 MHz. It sits at the boundary between HF and VHF behaviour, so most of the time it behaves like VHF and reaches only line of sight. Then a sporadic E patch forms and it suddenly delivers strong signals over a thousand miles for twenty minutes. The unpredictability is the appeal, and it is genuinely dramatic when it happens.

Why is 17 metres quieter than 20?

Partly because it is a narrower band with fewer stations and partly because contest operation is not permitted there by band plan convention. That keeps the activity conversational rather than competitive. It is open worldwide in daylight under most conditions, so it is an excellent band for a long relaxed contact.

Can I use 10 metres when solar activity is low?

Occasionally. F layer propagation on 10 metres largely closes at solar minimum, but sporadic E in the warmer months still produces openings over 500 to 1,500 miles, and those can be very strong. It is also worth watching because 10 metres is where the improvement shows first when the cycle turns upward.

Keep going

Related on this site

Keeping your own cut lengths, SWR sweeps and exposure record? The Station Build & Antenna Planner is the paid version of these pages: 8 printable worksheets you fill in with your own numbers, plus the full PDF, $29.

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