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NVIS Band Conditions

FEMA Region 6 • Texas ARES • AF MARS 6th Comm Wing

Texas Oklahoma Arkansas Louisiana New Mexico
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📊 Critical Frequency (foF2)
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Optimal NVIS
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💡 About This Recommendation

The dashboard recommends frequencies based on current foF2 and empirical propagation data.

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📻 NVIS Band Status Real-time Analysis

Understanding NVIS Propagation

foF2 is the critical frequency — the maximum frequency that reflects vertically from the F2 layer. For NVIS (0-300 mile range), use frequencies below foF2. Rule: Optimal NVIS = 85% of foF2. Data priority: Direct ionosonde → Regional interpolation → GPS TEC → IRI model. WSPR badges show real-world propagation verification.

NVIS Band Selection by Time of Day

NVIS propagation is highly time-dependent. Use this guide for initial band selection, then verify with live data above.

Time (Local) Primary Band Secondary Notes
0600–1000 40m (7 MHz) 60m (5 MHz) Ionosphere forming — 80m absorption increasing
1000–1600 40m (7 MHz) 30m (10 MHz)* Peak D-layer absorption kills 80m; *30m near solar max only
1600–2000 40m / 60m 80m (3.5 MHz) Transition — 80m opening as D-layer fades
2000–0600 80m (3.5 MHz) 60m (5 MHz) 40m may skip over regional targets at night

60m (5 MHz) provides the most stable 24-hour NVIS path. Times approximate for Central Texas (EM10) latitude.

💡 Data Source Types:
  • foF2 Sources (Priority 1-4): KC2G/GIRO → IRTAM → GloTEC → IRI-2016 provide ionospheric critical frequency
  • Solar Data Primary: HamQSL/N0NBH provides solar indices (SFI, K-index, A-index, sunspots)
  • K-Index Fallback: NOAA SWPC provides K-index only if HamQSL fails (not a complete replacement)
  • Ground Truth: WSPR.live provides digital mode activity for band verification
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foF2 Source Comparison

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