Winter 2005 Issue

The Solar Hits Keep Coming
in Cycle 23


Major aurora and auroral-E openings occurred
in early November 2004. Here is WB2AMU’s report on how VHFers took advantage of
these conditions.


By Ken Neubeck,* WB2AMU

At the beginning of November 2004 a series of coronal mass ejections (CMEs) were observed coming from an active sunspot on the sun, resulting in a buckshot effect that happened to be Earth-directed. Indeed, even though we are on the downside of solar Cycle 23, with the overall sunspot count generally below 100 and the solar flux below 150, solar events are still occurring!

Major Aurora

As these events were Earth-directed, it was a matter of two days before the amateur radio bands were impacted by the subsequent geomagnetic activity. As expected, the impact of multiple CMEs on the Earth’s geomagnetic field severely reduced HF activity. However, VHFers rejoiced at the potential aurora activity, and they were not to be disappointed.
The impact on the planetary K-index was noticeable over a three-day period, with the following three-hour intervals being recorded beginning at 0000Z:
November 8: 9 9 9 8 6 3 4 5
November 9: 6 6 5 7 6 7 8 7
November 10: 8 8 9 9 7 6 5 4

I was scheduled for a trip to Las Vegas with my XYL on November 8th, so I was busy packing, yet keeping an eye on the 6-meter chat page of DXer.info for any reports of aurora. When the reports started coming in, I took some time out to work stations on 6 meters from my location on Long Island, New York.

Signals on 6 meters were very strong, and I was hearing stations farther west than I normally do during an aurora opening. I was able to work KB8U in EN71 and NN9K in EN41, along with many other grids closer to me. At times some of the signals from the 8 and 9 call areas of the U.S. seemed to exhibit traces of auroral-E and were changing between aurora tones and auroral-E tones.
 

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