Solar-Terrestrial Snapshot LIVE IMAGE FROM HAMQSL

The image below is fetched live from HamQSL / N0NBH when the network is available. Everything else on this page (band-behaviour tables, interpretation notes) is static reference material that does not update automatically.

Embeds and links from public sources (N0NBH / HamQSL, NOAA). Refresh the page for latest images.

N0NBH Solar Data

Live image could not be loaded (CORS or offline).

Open HamQSL Solar Page
How to read
SFI
Higher = better HF
K-index
0–3
Quiet
K-index
4–5
Unsettled
K-index
6+
Storm

Typical Band Conditions (rule of thumb)

BandDayNightNotes
160 / 80 mPoor–FairGood–ExcellentNight DX, high noise by day
40 mFairExcellentWorkhorse regional + DX
30 / 20 mGood–ExcellentGoodPrime DX bands
17 / 15 mExcellent (high SFI)FairSolar-cycle dependent
12 / 10 mExcellent (high SFI)PoorDaytime only when open
6 mEs / F2 openingsRareSporadic-E summer, F2 peak cycle

These are generalizations. Real openings depend on path, time, power and antennas.

PSKReporter

Live digital-mode reception reports worldwide.

Reverse Beacon Network

CW & RTTY skimmer spots in near real-time.

WSPR Maps

Weak-signal beacon paths and heatmaps.

VOACAP Online

Classic path-prediction engine.

prop.kc2g.com

MUF / foF2 maps and effective SSN.

N0NBH / HamQSL

Full solar panels, MUF tools and banners.

Gray-line tip

Propagation is often enhanced along the gray-line (terminator). Check a gray-line map at sunrise/sunset for long-path or unusual openings on the lower bands.

Read the indicator before choosing a band

Use the solar and propagation indicators as planning inputs rather than guarantees of band openings. Compare the indicators with current on-air reports and your own observations.

Why local conditions may disagree

Propagation depends on time, location, path geometry, season, geomagnetic conditions and the ionosphere. A single index cannot describe every path.

Cross-check before changing bands

Combine forecasts with cluster reports, beacons and recent operating experience before making a band-choice decision.

Interpreting the numbers STATIC REFERENCE

Propagation indicators are useful because they describe the state of the ionosphere rather than the performance of one particular antenna. Solar flux, sunspot activity and geomagnetic indices can help explain broad HF trends, but none of them directly guarantees a good path between two stations. Frequency selection matters: a band that works well for one path can be poor for another because the ionosphere changes with latitude, local time and solar illumination. Treat indices as context and combine them with current reception reports, beacon observations and your own measurements. A strong signal report can also be misleading if local noise is low at one station but high at the other. When planning a contact, choose a likely band, check the current conditions, test the path and move between bands when the first choice is weak. The calculator and reference material are therefore best used as a decision aid rather than as a promise of propagation.

A useful habit is to record the band, UTC time, signal report and propagation indicators for successful and unsuccessful contacts. Over time those observations become more informative than any single index because they show how your own station behaves under changing conditions.

Next step in the workflow

Use the calculation as a starting point, then move to the tool that answers the next practical question.