f HF Propagation Today

↑ HF Propagation Today

This page is part of the project "Understanding HF Propagation."
by Doron Tal, 4X4XM
 

Useful charts showing HF propagation today

  1. DXView—online activity map on 1.8 MHz to 50 MHZ
  2. MUF 3000 km mapDX propagation conditions for a 3000 km path
  3. A dynamic global HF Score for the high bands, 17m, 15m, 12m, and 10m
  4. T index mapregional fluctuaions compared to the last month global average


↑ The following online activity map designed by Jon Harder, NG0E shows real-time QSOs on 11 HF bands.

DXview - real-time map of radio hams activity
Figure 1: DXView of real-time QSOs, on a selected band, or on all bands
First click on the above map; then you may click on "Perspective" filling in your QTH location.

The DXView map helps identify open bands and communication modes based on real-time activity from the last 15 minutes. It compiles data from online sources: WSPRnet, RBN (CW, FT4, FT8), and DX Cluster. Signal-to-Noise Ratio (SNR) data determines if a path supports SSB (SNR > 10 dB), CW (SNR > -1 dB), or only digital modes (decoding down to about -28 dB SNR). The DXView website provides a guide on interpreting the map and selecting band colors.


↑ Propagation DX map The solar radiation and space weather affect HF propagation.
The following MUF 3000 km map designed by Andrew, KC2G, shows near real-time HF propagation conditions for a 3000 km path.

MUF3000 map
Figure 2: MUF 3000 km map designed by Andrew, KC2G
1. How to use this online map 2. Additional notes 3. Animated map

↑ Global HF Score
↑ Real-time propagation conditions by HF Activity Group
The bar above represents the global "HF score" in the high bands (17m, 15m, 12m, and 10m), with values ranging from 0 to 100.
It updates every 5 minutes based on global propagation indices.
Regional or local conditions may be quite different.
The HF score graph below illustrates fluctuations over time, reflecting varying levels of solar activity and geomagnetic activity. Peaks indicate favorable (global) propagation conditions, while dips signify less optimal conditions; Updates every 5 minutes.
The red line provides a 48-hour trend for reference.
Graph is based on data from NOAA SWPC , NASA GOES .
Figure 3: HF Score of 10-17m bands, courtesy HF Activity Group

Rapid changes in the global HF propagation conditions are primarily due to variations in the ionosphere, which is affected by solar activity and geomagnetic storms. These factors influence the ionosphere's ability to bounce skywaves, leading to changes in signal strength, signal-to-noise ratio, coverage, and the potential for skip zones. Read more.


↑ Regional fluctuations
Below, see complex regional changes of the propagation conditions referred to the global average. The T index indicates the recent regional conditions (15 minutes) in relation to the worldwide average from the preceding month.

T Index Map
Figure 4: Online T Index Map courtesy of ASWFC; Updates every 15 minutes

Click on Figure 4 to read explanations.


The HF Propagation page provides detailed overview and tutorials on additinal aspects of HF propagation.


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