RF propagation in the HF (High-Frequency) band can be affected by two types of
D-Region absorption event - in extreme conditons either type can
produce a Radio Blackout:
[more]
- At lower latitudes, X-rays from solar flares can cause a Short
Wave Fade (SWF) event - SWF events can only occur on the daytime side of
the Earth and persist for the duration of the flare (tens of minutes to
hours).
A prediction of the effect of this type of event is shown in the SEC HAF Plot
(upper plot, left panel); this shows the highest affected frequency
based on flare intensity and user location - see also IPS
ALF Plot;
the X-ray lightcurve (lower plot, left panel) shows current conditions.
Alerts related to SWF events (produced by IPS)
are also shown (upper table, left panel).
[IPS ALF - last major flare]
- In the polar/auroral zone, protons precipitating down the Earth's
magnetic field lines can produce a Polar Cap Absorption (PCA) event -
PCA events start within 15 minutes to 2 hours of the flare and last anywhere
from about an hour to several days (with an average of around 24 to 36 hours).
The intensity of proton precipitation (upper plot, right
panel) is a good pointer to the likelyhood of this type of event -
also see the proton lightcurve (lower plot, right panel) for
current conditions.
[Polar Maps]
[IPS PCA Report]
[IPS - Realtime Riometer]
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