Ham Radio Propagation Explained

How HF signals travel around the world and how to read the numbers

The Ionosphere — Your Mirror in the Sky

HF radio propagation relies on the ionosphere, a layer of electrically charged particles (ions and free electrons) between 80 km and 400 km above Earth's surface. Solar ultraviolet radiation ionizes atmospheric gases, creating layers that can reflect radio waves back to Earth. This is how a signal from Tennessee can reach Europe or Japan on frequencies between 1.8 and 30 MHz.

The Key Numbers

Solar Flux Index (SFI)

Measures solar radio output at 10.7 cm. Range: ~65-300+. Higher = more ionization = higher bands open.

Below 80
Poor — 40m and below only
80-150
Fair — 20m reliable, some 15m
Above 150
Good — 15m/12m/10m open

Sunspot Number (SSN)

Count of visible sunspots. Correlates with SFI — more sunspots = more solar output = better ionization. The solar cycle is approximately 11 years. We are currently near the peak of Solar Cycle 25.

Maximum Usable Frequency (MUF)

The highest frequency that will be reflected by the ionosphere for a specific path. If the MUF between you and Europe is 21 MHz, then 15m (21.0-21.45 MHz) will work but 10m (28 MHz) won't. The MUF changes throughout the day, peaking around local noon when solar ionization is strongest.

Our Propagation Dashboard shows real-time MUF contour maps from KC2G PropNET, updated every 15 minutes.

Kp Index (Geomagnetic Activity)

Measures magnetic field disturbance on a 0-9 scale. Lower = calmer = better HF. Kp above 4 degrades polar paths. Kp above 5 is a geomagnetic storm that can black out HF entirely. Read our detailed Kp Index Guide.

Band-by-Band Guide

BandBest ForWhen It's Open
160mRegional to continental DXNight only. Best in winter. Very sensitive to noise and Kp.
80mRagchewing, nets, regional DXEvening through dawn. Trans-Atlantic possible in winter nights.
40mAll-purpose workhorseRegional daytime, DX at night. Reliable almost always.
20mDX kingDaytime, worldwide. Open most of the day during high solar activity. The most popular DX band.
15mDX when conditions are goodNeeds SFI above ~100. When open, excellent DX with lower noise than 20m.
12mDX, less crowdedSimilar to 10m but with WARC band allocations. Less traffic.
10mDX + Sporadic-ENeeds high SFI (>150) for F2 skip. Sporadic-E in summer opens it for regional contacts regardless of solar activity.

The Ideal Recipe

For the best HF DX conditions, you want:

  • - High SFI (above 150) — strong ionization supports higher bands
  • - Low Kp (0-2) — stable magnetosphere, no disruption
  • - Low solar wind speed (below 400 km/s) — no incoming disturbances
  • - High RBN spot count — confirms real-world band activity matches theory