PropDeck — HF propagation operations dashboard for amateur radio

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Open the ⚙ gear any time to fine-tune layers, filters, WSJT-X, your ADIF log, and more. Propagation paths now center on your QTH.

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Solar Data

Solar Data Legend

SFI (Solar Flux Index)

Measures solar radio noise. 70 is low, 150+ is excellent for HF propagation.

A-Index (Daily Average)

Geomagnetic activity. < 10 is quiet,> 30 is active/unstable.

K-Index (Current State)

Quasi-logarithmic measure of activity. 0-2 is quiet, 5+ is a storm.

SN (Sunspot Number)

Number of sunspots. Higher counts correlate with better ionization.

Solar Wind Speed

24h timeline of solar wind plasma speed from NOAA DSCOVR/ACE satellite. High-speed streams compress Earth's magnetosphere and drive geomagnetic storms.

Speed Bands

Background bands show conditions:
Slow < 400 | Nom 400–500 | Elev 500–700 | High > 700 km/s

HF Impact

Sustained speeds above 500 km/s often trigger G-scale geomagnetic storms, degrading HF propagation — especially at high latitudes.

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Space Wx

NOAA Space Weather Scales

R (Radio Blackouts)

Caused by X-ray emissions. Affects HF radio propagation on sunlit side.

S (Solar Radiation Storms)

Caused by proton events. Affects HF radio in polar regions.

G (Geomagnetic Storms)

Caused by CME/Solar Wind. Affects HF globally, can cause aurora.

Scale (0-5)

0: None, 1: Minor, 2: Moderate, 3: Strong, 4: Severe, 5: Extreme

GOES X-Ray Flux

24h timeline of solar X-ray flux from GOES satellite (0.1–0.8 nm long channel). Rising flux indicates a solar flare in progress.

Flare Classes

Background bands show classification thresholds:
B < 10⁻⁶ | C 10⁻⁶–10⁻⁵ | M 10⁻⁵–10⁻⁴ | X > 10⁻⁴ W/m²

Badge (e.g. C3.2)

Current classification and sub-level. M/X flares cause HF blackouts within minutes — watch for rapid rises.

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Map Control

Map Overlay Guide

MUF-RT (Maximum Usable Frequency)

Real-time calculation of the highest frequency for a 3000km hop. Essential for identifying DX openings on 10m-20m bands.

foF2 (Critical Frequency)

The highest frequency at which a signal is reflected vertically. Key for NVIS and local regional communication on 40m-160m.

MUF-VCAP (Variable Coverage)

High-fidelity VOACAP model using your custom Power, Mode, and Antenna. Simulates real-world signal probability at your location.

DRAP (Absorption Map)

D-Region Absorption Map. Visualizes HF signal attenuation caused by solar X-ray flares and proton events.

Aurora (Borealis/Australis)

Real-time visualization of the Auroral Oval. Indicates where trans-polar paths may be blocked or enhanced by scatter. The Aurora pill shows the global peak probability; a trailing ↑ (amber G1–G2 / red G3+) warns a geomagnetic storm is forecast within 24h.

PSK Heat (Live Reception)

Magenta heat of where signals are actually being heard right now, from the live PSK Reporter firehose — brighter means busier. Real observed activity, separate from the predicted coverage maps. Use the 🌐/📍 scope toggle in the widget header (left of the collapse arrow) for worldwide vs your local footprint.

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