KR4BJN

EM87 | Eastern Kentucky, USA

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HF Band Conditions

Solar Chart

Solar-terrestrial data

  • A higher Solar Flux Index (SFI) means more radio “fuel” from the Sun, better chances of long-range HF communications.
  • More sunspots (SN) generally mean higher solar activity, which enhances the ionosphere's reflecting power.
  • Geomagnetic indices (K-index, A-index): These measure how calm or disturbed Earth's magnetic field is. Lower values = better for radio propagation; higher values = storms/disruptions.
  • X-ray flux, 304 Å (angstrom) UV radiation, particle flux (protons/electrons), etc.: These indicate more subtle or advanced effects (like absorption in the lower ionosphere, or auroral disturbances). If any of these climb, propagation may degrade.

If many of the values are in the “good” range and the band-condition ratings show “Good”, then it's a favorable time for radio operators to make long-distance contacts.

If the geomagnetic or particle indices are high (indicating a disturbance or storm), even a high solar flux might not translate into good propagation — because disturbances can upset the ionosphere's "mirror."

The conditions vary with time (day/night), frequency band, and geographic region, so what's shown is a global/average reading (local conditions might differ).

MUF Map

Worldwide maximum usable frequency map

  • MUF stands for Maximum Usable Frequency — the highest radio frequency at which a short-wave (HF) radio signal can still be reflected by the ionosphere and make long-distance (“skip”) contacts.
  • In simple terms: Above the MUF value, the signal goes through the ionosphere into space, rather than being bounced back to Earth.
  • MUF is path- and time-dependent; what works between two locations at one hour may not work at another.

The map shows colors or contours representing the current estimated MUF for radio paths over wide regions. If a region shows, e.g., 25 MHz, that means signals up to about 25 MHz might successfully propagate that distance via the ionosphere.

A higher MUF number means the ionosphere is more ionized (usually due to sunlight and solar activity), so higher-frequency HF bands (e.g., 15 m, 12 m, 10 m) may be usable for long-distance contacts.

A lower MUF means conditions are weaker, so you'll likely need to use lower-frequency HF bands (e.g., 40 m, 80 m) for reliable contacts.