Sunspot cycle 24 began slowly subsiding in 2014. Even so, it will still produce some good DX opportunities for a few years. This page has information on solar activity for the ham radio DXer.
The three-month sunspot moving average hit its lowest count in August 2008.
No "significant" sunspot activity was observed ... until a sunspot persisted for five days at high latitudes before disappearing on June 4 2009.
Cycle 24 was born!
The sun's activity provided ham radio operators all over the world with a number of
good to excellent signal propagation conditions. Now that it's over the top, we have to watch the sun's activity more closely to make the most of it.
A considerable amount of information on solar-terestrial data and propagation conditions is available on N0NBH website. It is definitely worth a visit.
I must tell you that I find N0NBH's Web site one of the most informative sites on solar radiation and the sun's influence on signal propagation. If you are at all interested in acquiring a better understanding of the sun's impact on our hobby, this is one site I recommend without hesitation.
Here is the latest picture showing sunspot activity!
An international panel of experts predicted, in June 2009, that Solar Cycle 24 would likely not produce a smoothed sunspot number exceeding 90!
It laboriously reached a peak of 81.9 in April 2014!
In comparison, cycle 23 had produced a maximum smoothed sunspot number around 160 in 2001 which, in itself, was less than the maximum observed during each of the two previous cycles.
In other words, we are told not to expect too much out of solar cycle 24. The experts were right.
But, hey! It's so quiet on HF during a solar minimum that any sunspot activity, and its beneficial effect of the "F" layer, are very welcome indeed :-)
Here is the latest news on sunspot activity.
73 de VE2DPE
7, Rue de la Rive, Notre-Dame-des-Prairies, Québec, Canada J6E 1M9
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