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Guide · shortwave / HF

Shortwave (HF)

This is the heart of amateur radio. On the bands from 160 to 10 metres the signal reflects off the ionosphere and returns to Earth hundreds or thousands of kilometres away — without the internet, without repeaters, without satellites. With a length of wire strung between trees and a handful of watts you can talk to the other side of the world. This guide is your map: bands, propagation, antennas, modes, equipment and your first QSO.

160 – 10 m 1.8 – 29.7 MHz SSB · CW · FT8 DX worldwide
A radio amateur erecting a mast with a Yagi antenna on a snow-covered mountain summit
portable operation · photo: brewbooks / Wikimedia Commons, CC BY-SA 2.0
Why it’s addictive

The world within reach of a length of wire

Shortwave is the only part of the spectrum where an ordinary ham with a home antenna can regularly work other continents — thanks to physics, not infrastructure.

01

Global reach

Ionospheric reflection (a so‑called hop) carries the signal thousands of kilometres. A single QSO can link Warsaw with Japan or South America.

02

Low power, big results

In good conditions even a few watts (QRP) and a simple antenna are enough for long‑distance contacts. It’s propagation and the antenna that count, not the amplifier.

03

Physics in action

Bands “breathe” with the time of day and the Sun’s cycle. The same antenna is silent one moment and opens to the whole globe the next — and it’s that hunt for conditions that gets you hooked.

04

Contests and awards

DX, contests, operating from summits (SOTA) and parks (POTA), QSL confirmations and awards like DXCC — there’s plenty to compete for and to collect.

Band map

HF bands and their character

Every band has its own temperament — some come alive at night and locally, others in the day and worldwide. Here’s a brief guide (IARU Region 1 / Poland band plan).

Low bands — “night‑time”

160 · 80 · 40 mLF/MF vibe

Absorbed by the D layer during the day, they come alive after dark. The domain of national and European QSOs, and of winter DX. They need large antennas, but have a distinctive, “warm” feel.

BandRange · character
160 m1.810–2.000 MHz · night‑time, demanding, “topband”
80 m3.500–3.800 MHz · evening QSOs, national/EU
40 m7.000–7.200 MHz · versatile: daytime regional, night‑time DX

High bands — “daytime”

20 · 15 · 10 mDX

They open in the day and carry DX worldwide. The higher the band, the smaller the antenna and the more it depends on solar activity. 20 m is the king of DX — almost always open.

BandRange · character
20 m14.000–14.350 MHz · prime for DX, active all day
15 m21.000–21.450 MHz · excellent with high solar activity
10 m28.000–29.700 MHz · can “explode” (Es, cycle peak)
i

WARC bands (30 m: 10.1 MHz · 17 m: 18.1 MHz · 12 m: 24.9 MHz) are quieter, narrow bands without contests — 30 m is for CW and digital modes only. Always check the detailed allocations, mode segments and power limits in the current PZK (the Polish Amateur Radio Union) / IARU R1 band plan.

How signals travel far

Ionospheric propagation

All the HF magic happens a few hundred kilometres above your head — in the Sun‑ionised layers of the atmosphere.

The ionosphere in brief

  • Reflection, not line‑of‑sight. A wave sent upwards reflects from the F layer and returns to Earth far away — that’s a “hop”. Several hops = intercontinental contact.
  • Day versus night. By day the D layer absorbs the low bands (160/80 m go quiet) but boosts the high ones (20/15/10 m). After dusk it’s the other way round — the low bands come alive.
  • The Sun rules. The more sunspots (high SFI), the higher the MUF — the maximum usable frequency. At the peak of the cycle, 10 m can be open worldwide.
  • Grey line. At dawn and dusk, along the boundary between day and night, propagation on the low bands can strengthen exceptionally — a good time for DX.
  • Sporadic‑E. In summer the E layer gives sudden, strong openings on 10 (and 6) m — brief but spectacular.
A large amateur radio station with multi-element directional antennas on a mast, bird’s-eye view station with HF beam antennas · photo: Wikideas1 / Wikimedia Commons, CC0
The most important part

Antennas for shortwave

On HF, the antenna makes a bigger difference than power. A good antenna and 100 W will beat a poor antenna plus an amplifier. Where to start?

◇

Dipole 1/2 λ

A classic and the standard. A length of wire, centre‑fed, strung between two points. Cheap, effective, easy to build for 40/20 m.

▲

Vertical (GP)

A vertical radiator with radials. Takes little horizontal space, radiates well at low angles — great for DX.

━

Long wire + ATU

A long wire and an ATU (tuner) to match it on many bands. The simplest way to operate “on everything” from a small garden.

◎

Magnetic loop

A small loop for a balcony and tight QTH. Compact and quiet on receive, at the cost of narrow bandwidth (needs retuning).

When to go for a beam

  • A Yagi for the high bands. On 20/15/10 m a directional (tri‑band) antenna gives real gain and rejects interference from other directions — the DXer’s dream.
  • Needs a mast and a rotator. You must turn it towards the other station and get it up high. On the low bands it becomes enormous — that’s why wires rule there.
  • Wire first, then a beam. Start with a dipole or a vertical — you’ll learn the bands and propagation for less money, and add a beam once you’re hooked.
  • SWR and tuning. Every antenna is tuned for minimum SWR on the band; an ATU helps “tweak” the match.
A multi-element Yagi beam for the HF bands on a portable mast, against the sky HF Yagi beam · photo: Lz1aat / Wikimedia Commons, CC BY-SA 3.0
How we talk

Modes on HF

The same transceiver lets you operate by voice, with a key or via a computer — each mode has its own character and strengths.

🎙

SSB (voice)

Voice contacts. Below 10 MHz use lower sideband (LSB), above use upper (USB). The easiest way in — grab the mic and call CQ.

·−

CW (telegraphy)

Morse code. Narrow bandwidth and excellent readability with weak signals — with low power you’ll get further than on voice. Practise with the trainer →

▦

FT8 / digital modes

The computer encodes the signal so it gets through noise your ear can no longer hear. It excels in poor conditions and with QRP.

≋

RTTY · AM · more

Radioteletype (RTTY), nostalgic AM, PSK31 and much more. HF is a playground for modes — plenty to explore for years.

Where to start

Gear to get started

An HF setup is simpler than it seems. The biggest investment isn’t the radio, but the time spent on a good antenna.

Basic HF toolkit

  • HF transceiver — covering 160–10 m; 100 W output is standard. Classic used rigs can be a great, inexpensive start.
  • Antenna + feedline — a dipole or a vertical and good coax (calculate the loss in the cable loss calculator).
  • Antenna tuning unit (ATU) — matches the antenna on different bands; many transceivers have one built in.
  • SWR/power meter — checks the antenna is tuned and that the radio is operating safely.
  • Power supply and earthing — a steady 13.8 V and solid station earth for safety and a clean signal.

Start by listening — for free

Before you pass the exam, just listen. An SDR receiver (even an online WebSDR) will show you how the bands open and close over the day. You’ll learn to recognise modes, callsigns and the rhythm of QSOs — it’s the best training before your first “CQ”.

You don’t need any licence to listen. To transmit on HF you need an operator’s certificate and a radio licence (exam at UKE — the Polish Office of Electronic Communications) — full access to the shortwave bands comes with a Class A certificate.

Step by step

First HF QSO

Voice on 40 or 20 m — the easiest. Here’s the whole flow of a first long-distance contact.

1

Find an open band

Tune across 40 and 20 m. Hearing lots of stations = the band is alive. Rule of thumb: by day aim higher (20/15 m), in the evening lower (40/80 m).

2

Listen first

Pick a free frequency and make sure no one is using it. Ask before you call.

“Is the frequency in use? This is SQ5CBA”
3

Call CQ (or reply)

Make a general call or answer someone calling CQ. Use the phonetic alphabet — spell your callsign clearly.

“CQ CQ, this is Sierra Quebec Five Charlie Bravo Alfa, calling CQ”
4

Exchange reports

Give your callsign, RST report (readability and strength), name, QTH and locator. Note the same from the other station.

“Report 59, name Filip, QTH Warsaw, locator KO02”
5

Finish and log it

Say thanks, sign off with the classic “73” and enter the contact in your log. You can send QSL confirmation electronically.

“Thank you for the QSO, 73! SQ5CBA”
✓

Tip: the first time is the hardest. Start by answering other people’s CQ, rather than calling yourself — it’s easier to join an ongoing contact. And if voice makes you shy, try FT8: the computer handles the whole exchange and you learn the bands and propagation without mic stress.

Where it leads

Hunting DX

Once you catch the rhythm of the bands, the real game begins: chasing distant and rare stations.

🌍

DX and DXCC

“DX” is a distant station. For confirmed QSOs with different countries you earn the legendary DXCC award — a lifetime collection.

⛰

SOTA and POTA

Operating from summits (Summits on the Air) and parks (Parks on the Air) — combining amateur radio with hiking and the outdoors. Light gear, big thrills.

📣

Pile-up and split

When a crowd is calling a rare station, it operates “split” — listening slightly off its transmit frequency. The trick is to hit its window.

🏆

Contests

Weekend contests are a crash course in operating: hundreds of QSOs, time pressure and bands full of life. A great way to grow quickly.

Cheat sheet

Mini-glossary for HF

shortwave / HF
shortwave, the 1.8–30 MHz bands (160–10 m)
DX
a distant or rare station; “doing DX” = chasing long-distance contacts
QRP
low-power operating (≤5 W CW / 10 W SSB) — a sport in its own right
Hop
a single reflection of the wave from the ionosphere back to Earth
MUF
the highest frequency that will still be refracted back by the ionosphere
SFI / sunspots
indices of solar activity — the higher they are, the better the high bands
Grey line
the dawn/dusk zone with exceptionally good low-band propagation
Sporadic-E
sudden summer openings on 10/6 m via the E layer
ATU / tuner
an antenna tuning unit matching the antenna to the radio
SWR
standing wave ratio — a measure of antenna matching (aim: close to 1)
RST
report: readability, strength (and tone for CW)
Split
transmitting and receiving on different frequencies (working a pile-up)
Pile-up
a crowd of stations calling one rare station at once
DXCC
award for confirmed contacts with different countries/territories
Locator
Maidenhead grid square (e.g. KO02) — station location
73
best regards — the classic way to end a QSO
Next step

Learn CW

On HF, CW is a superpower — with weak signals and low power you’ll get the furthest with it. Practise the characters with the interactive Morse trainer, then visit the guide to the 2 m and 70 cm bands.