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Steve White G3ZVW

 

6m activity from G3ZVW in October 2003


With the Sporadic-E season well passed, the band was pretty-much dead for the whole of the month. However, on the 29th a coronal mass ejection from the sun resulted in some spectacular auroral conditions.

By 1700 the band was open to many northern european countries.
During the course of the evening I used a fair mix of SSB and CW to work LA, GM, F, OH, ON, G, EI, GW, PA, OZ, SM, ES and DL. Squares worked were: JO28 IO87 IN94 KP12 JO89 JO01 IO80 IO91 IO97 IO86 IO88 IO52 JO03 JP70 IO81 IO91 IO63 JO32 JO55 JO54 IO90 IO81 IO94 JO01 KO29 JO45 JO56 JO22 JO65 IO86 IO93 JO33 JO22 JO45 JO21 IO67

Propagation was "interesting", and by that I mean that some stations nearby were received completely via the aurora (e.g. G3ZRH, who lives in Brentwood), whilst some distant stations (e.g. GM8LFB, SM4XIP and ES2RW) had little or no hint of the aurora about them. Some QSOs were auroral in one direction and non-auroral in the other - very stange indeed!

On the 30th a much less intense aurora brought in a few weak stations. Interestingly, at 2200 an SM7 was romping in here at 5/9+ with no hint of auroral propagation being present on his signal.

What do auroral signals sound like?
On SSB, signals sound as though they have gone through a mincing machine. Speech becomes extremely gurgly and difficult to understand. Auroral contacts often take place using words which are spoken slowly, especially if signal levels are weak. Contacts are short and phonetics used throughout. On CW, the pure tone that we are accustomed to is completely gone and replaced by a hissing sound.

Because of the effects that an aurora has on signals, thay are reported in a different way. "57A" might be typical, where "5" is the readability, "7" is the signal strength and "A" is for Aurora. The same scheme applies to CW and SSB.

The reason auroral signals sound so different is that they are being reflected by an ever-changing and rapidly-moving reflector (the ionised gases in the aurora). This results in multi-path reflections and the introduction of doppler shift into the signals.

Steve, G3ZVW


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