Winter 2004 Issue

Fall 2003 Aurora Events and More

The hits of solar Cycle 23 just seem to keep on coming.
Here is WB2AMU’s report on the significant happenings
of October and November last year.


By Ken Neubeck, WB2AMU

As solar Cycle 23 progresses toward its conclusion, both the sunspot count and the solar-flux values continue to ratchet lower than they were a year ago. However, recent solar activity suggests that this cycle still lives, in the process providing unexpected excitement on the VHF ham bands. What follows is documentation of some of the excitement that took place this past fall.

October 2003

On October 28, 2003, at 1048 UTC, a major solar-flare explosion was observed erupting from designated solar region 10486, at the high level of X17 (see the accompanying LASCO image photograph by NOAA). At the time, the level of the solar flare was the third largest recorded in the last two decades. The timing of the flare was such that the sunspot area from where the flare originated was in a geo-effective area pointed toward Earth. Also in contrast to previous solar flares and coronal mass ejections (CMEs), the wave action from this flare was traveling at exceptionally high speeds, in excess of 1200 km/sec.

With the high speed and the geo-effective direction, impact was expected during the day of October 29. While HF operators were expecting radio blackouts and fading up to 30 MHz, VHF operators had expectations of major aurora events if the planetary K value was to reach or exceed 7. Typically, such events take about two days to travel from the sun to the Earth, but the exceptionally high speed of this particular event caused it to arrive in only one day!

Impact took place at around 0900 UTC on October 29, and by 1200 UTC aurora openings were being observed on 6 meters in northern Europe. However, with the all-important Bz value (the magnetic field intensity in the all-so-important north-south direction) showing magnetic-field intensity not quite favoring southward, it took a while after impact for activity to show up in the US. By 1900 UTC aurora appeared on both the 6- and 2-meter bands in the US and Canada. The opening was fairly strong, as it reached into a number of the southern US states. It was during this time that the three-hour planetary K value reached a peak of 9.

From my QTH on Long Island I observed strong aurora signals on 6 meters from the neighboring grid squares in Connecticut, Massachusetts, New Jersey, Pennsylvania, and Delaware. I also heard some signals on 2 meters from the Virginia area. There were many visual observations of aurora in the US, although unfortunately my area was heavily overcast, which blocked viewing.

 

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On October 28, 2003, at 1048 UTC, a major solar-flare explosion was observed erupting from designated solar region 10486, at the high level of X17. (LASCO image photograph by NOAA)