PropDeck — HF propagation operations dashboard for amateur radio

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Solar Data

Solar Data

Live numbers for the two big HF drivers: how much the sun is fueling the ionosphere (SFI / SSN), and how much Earth’s magnetic field is stirring it up (A / K, plus solar wind + IMF Bz / Bt on the storm side). Small arrows next to each value are 24h trend (up / down / flat), not absolute quality.

SFI (Solar Flux Index)

10.7 cm solar radio flux — a stand-in for the UV that ionizes the F layer (the layer that bends most HF DX). Higher SFI usually means a higher MUF and better chances on 15 / 12 / 10 m. Rough guide: ~70 solar-min / weak, ~100 usable, 150+ excellent for the high bands.

SSN (Sunspot Number)

Count of sunspots. Tracks with SFI across the solar cycle: more spots → richer ionosphere → stronger high-band openings. Changes slowly day to day; use it for “where are we in the cycle?” more than hour-to-hour decisions.

K-Index (now)

How disturbed Earth’s magnetic field is right now (0–9, updates every few hours). Quiet K leaves paths alone. Rising K stirs the F layer: polar and high-latitude paths die first, signals flutter (auroral sound), MUF can drop or go unreliable, and lower bands (160 / 80 / 40) absorb more on high-lat paths. Mid-latitude short skip often holds up longer.
0–2 quiet · 3–4 unsettled · 5+ storm

A-Index (daily)

Same idea as K, averaged over the whole day on a linear scale. Best for “was today stormy?” and recovery: A can stay elevated for hours after K falls while the ionosphere settles.
<10 quiet · 10–30 unsettled · >30 active / stormy

Bz (IMF north–south)

Interplanetary magnetic field component in nT (GSM). This is the coupling switch between solar wind and Earth’s magnetosphere: south (negative) couples well and, with elevated wind, is the classic geomagnetic-storm recipe; north (positive) couples poorly so fast wind often stays quiet. Arrow is the 24h change (more south = worse). When Bz has been south for a while and solar wind is elevated, the map may show an amber IMF SOUTH · STORM RISK banner as a heads-up before K / G rise.

Bt (IMF total)

Total interplanetary magnetic field strength in nT — how strong the field is, regardless of direction. Higher Bt means more magnetic energy available; pair it with Bz: high Bt + south Bz is a stronger storm setup than high Bt + north Bz. Arrow is the 24h change (rising = more field energy). Rough guide: <5 quiet, 5–15 elevated, >15 strong.

Quick read

High SFI + low K → good high-band day. High SFI + high K → lots of ionization but flaky paths (especially polar DX). Low SFI + low K → stable but limited openings. High wind + south Bz (especially with high Bt) → watch for a geomagnetic hit even if K is still quiet. Pair this with Space Wx for flares / blackouts (R scale) and the Conditions widget for per-band Good / Fair / Poor.

Solar Wind Speed

24h timeline of solar-wind plasma speed from NOAA DSCOVR / ACE (far upstream of Earth). Fast streams compress the magnetosphere and are a common reason K and A climb — and why aurora lights up. Watch the shape: a sharp jump often precedes a geomagnetic hit by hours.

Speed Bands

Background colors on the chart:
Slow < 400 | Nom 400–500 | Elev 500–700 | High > 700 km/s

HF Impact

Sustained speeds above ~500 km/s often feed G-scale geomagnetic storms (see Space Wx) when Bz is south. Expect degraded reliability on high-latitude and polar paths first; mid-latitude paths can still work. Wind alone is incomplete — confirm with Bz / Bt, rising K, and the G scale before writing the bands off.

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Space Wx

Space Wx

NOAA storm scales and live X-ray flux — the event side of space weather. Where Solar Data is the background (fuel vs quiet magnetic field), this widget flags flares, radiation storms, and geomagnetic storms that can kill a band in minutes or wreck polar paths for hours.

The R / S / G grid

Three storm types, four time columns: −24h (what already hit), NOW (current observed level), +24h and +48h (forecast). Numbers are NOAA severity 0–5 (blank / 0 = quiet). Watch both “is it happening now?” and “is something forecast?” — a rising +24h G is your heads-up before K climbs.

R — Radio Blackouts

Driven by solar X-ray flares. Hard X-rays jack up the D layer on the sunlit side of Earth within minutes — HF signals get absorbed (lower bands first: 160 / 80 / 40 hard hit; higher bands less so). Night-side paths often keep working. Tied to the GOES X-ray chart on the right (M1 ≈ R1, X1 ≈ R3, etc.). Blackouts usually last minutes to an hour after the flare peaks.

S — Solar Radiation Storms

Driven by energetic protons from big flares / CMEs. They dump into the polar caps and cause polar-cap absorption (PCA): HF over the poles can go dead for hours to days even when mid-latitude paths look fine. Less common than R or G; when S is up, avoid polar routes and high-latitude DX.

G — Geomagnetic Storms

Driven by CMEs and fast solar wind slamming the magnetosphere. Same physical storm family as high K / A in Solar Data and a lit-up aurora oval: F-layer chaos, flutter, depressed or unreliable MUF, worst on polar and high-latitude paths. Unlike R (minutes, sunlit only), G can last many hours and hit day and night.

Scale (0–5)

0 none · 1 minor · 2 moderate · 3 strong · 4 severe · 5 extreme. For operators: 1 is “noticeable,” 3+ is “plan around it,” 5 is rare and nasty. Color intensity in the cells tracks severity.

Quick read

Spike on X-ray / R rising → expect sunlit HF fade (check the DRAP map). G climbing or forecast → watch K and aurora; polar DX first to go. S up → polar paths toast. All quiet → trust Solar Data (SFI / K) and Conditions for the normal picture. Storm banners on the map jump you here when something is active.

GOES X-Ray Flux

24h timeline of solar X-ray flux from GOES (0.1–0.8 nm long channel). A rapid rise is a flare in progress — that is the live feed behind the R scale. Flux falls after the peak; D-layer absorption eases as it does.

Flare Classes

Background bands on the chart (each letter is 10× the previous):
B < 10⁻⁶ | C 10⁻⁶–10⁻⁵ | M 10⁻⁵–10⁻⁴ | X > 10⁻⁴ W/m²

Badge (e.g. C3.2)

Current class and sub-level (C3.2 = C-class, 3.2× the C threshold). B/C are common background. M and especially X can cause R-scale HF blackouts within minutes on the day side — watch for a steep climb, not just a high plateau. Pair with the DRAP overlay to see where absorption is worst right now.

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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.

VCAP-BEST (All-band Reliability)

The real VOACAP (ITS HF) engine, run live for your location with your Power, Mode, and DE/DX antennas, with live sporadic-E, then overlaid with live storm/flare effects when those feeds are available. Shows the most reliable band at your chosen reliability threshold; pick a single band to see its 0–100% reliability. Configure antennas, noise, reliability, antenna aim, and sporadic-E in Settings → VOACAP.

DE Antenna Aim (map handle)

When DE Antenna is a Wire or Beam type, a labeled aim graphic appears at your DE pin. BEAM (cyan) is the main-lobe direction VOACAP uses. For wire antennas, WIRE (amber) shows the physical wire run — broadside to the beam, not the same heading. Drag either tip to rotate; right-click the map for Aim antenna here / Aim antenna at DX pin. Isotropic and verticals are omnidirectional — no aim control.

Per-Band Reliability (160–10 m)

The band pills (160 / 80 / 60 / 40 / 30 / 20 / 17 / 15 / 12 / 10) each render VOACAP coverage for that one band — every point colored 0–100% by how reliably you can work it, on the same scale as the legend. Same engine and settings as VCAP-BEST, just a single band instead of the best one, so you can see exactly where, say, 20 m or 40 m is open right now.

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 globe / pin scope toggle in the widget header (left of the collapse arrow) for worldwide vs your local footprint — the same pair the Conditions widget uses.

Lightning (Blitzortung)

Live strikes from Blitzortung.org (CC BY–SA 4.0), fetched by the PropDeck server and polled by your browser — clients never open Blitzortung directly. Bolts flash in, age yellow to red, and fade over about two minutes (newest 200 on screen). The bolt icon left of Sats shows/hides the worldwide layer. Nearby activity toasts (within 100 km of DE) are under Settings → Map & Overlays → Alerts & Warnings; with those on, local bolts still draw in that bubble even if the worldwide layer is off.

Grid

Draws one world grid on the map: Lat/Lon graticule (15°, refining to 5°/1° with edge degree labels as you zoom), Maidenhead locators (fields, then 2°×1° squares as you zoom in), CQ zones, ITU zones, or the three ITU Regions. Off by default; works in every projection.

Pwr / Mode / Toa (VCAP inputs)

These three dropdowns feed the live VOACAP engine used by VCAP-BEST and the per-band reliability pills. Changing any of them re-runs the overlay for your DE. Antennas, aim (main beam / wire run), noise, reliability threshold, and sporadic-E live under Settings → VOACAP.

Pwr

Your transmit power in watts. Higher power raises predicted SNR and expands the reliable coverage footprint on the map.

Mode

Operating mode sets the required SNR for a path to count as reliable (e.g. WSPR and FT8 need less signal than SSB or AM). Pick the mode you actually run so the colors match what you can work.

Toa (takeoff angle)

Minimum takeoff angle VOACAP will consider. Lower values (e.g. >1°) include grazing low-angle DX paths; higher (e.g. >9°) favor shorter / higher-angle hops and match antennas that don't launch low. Default >3° is a solid all-round choice.

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