:Product: Weekly Highlights and Forecasts :Issued: 2001 Dec 19 2212 UT Highlights of Solar and Geomagnetic Activity 10 - 16 December 2001 Activity ranged from low to high levels during the period. High levels occurred on 11 and 13 December due to two major flares from Region 9733 (N14, L = 313, class/area Eki/560 on 12 December). Activity alternated between low and moderate levels during the rest of the period. Region 9733’s first major flare was an impulsive X2/2b at 11/0808 UTC, the second a X6/3b at 13/1430 UTC. The X6/3b flare was associated with a partial-halo CME. Region 9733 was large and magnetically complex through most of the period. It produced impulsive low-level M- and C- class flares as it gradually decayed following the X6 flare (for flare times, please refer to the Energetic Events or Optical Flares lists). The other sunspot group of interest was Region 9727 (S21, L = 020, class/area Eki/630 on 13 December), which produced isolated low-level M-class and C-class flares during the period. Region 9727 was in a gradual growth phase through 13 December, then stabilized as a large, magnetically complex group with a possible delta magnetic configuration in its northernmost trailer spots. It produced isolated subflares as it crossed the west limb on 15 December. Solar wind data were available from the NASA Advanced Composition Explorer (ACE) spacecraft for most of the period. A relatively weak high-speed stream associated with a positive-polarity coronal hole was observed during the last two days of the period. Velocities and temperatures were elevated during this time with intermittent “gusts” in the 500 to 600 km/sec range. There were no significant disturbances observed during the rest of the period. There were no proton events detected at geo-synchronous orbit. The greater than 2 MeV electron flux at geosynchronous orbit was at normal levels during most of the period. Geomagnetic field activity was at quiet to unsettled levels during most of the period. Forecast of Solar and Geomagnetic Activity 19 December 2001 - 14 January 2002 Solar activity is expected to range from low to moderate levels with isolated low-level M-class flares likely. Isolated major flare activity will also be possible during the period with the return of previously active longitudes. There will be a slight chance for a proton event during the period. The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal levels during most of the period. The geomagnetic field is expected to be at quiet to unsettled levels during the period. .