:Product: Weekly Highlights and Forecasts :Issued: 2001 Jan 16 2112 UT Highlights of Solar and Geomagnetic Activity 08 - 14 January 2001 Solar activity was at low to moderate levels during the period. The period began with activity at low levels due to isolated C-class subflares. Activity increased to moderate levels on 09 January due to an M1/1n flare from Region 9306 (N12, L = 055, class/area Fac/510 on 14 January). Region 9306, which showed gradual development through the period, was a large region with a moderate degree of magnetic complexity. Activity remained at moderate levels during 10 January by virtue of an impulsive M3/1n flare at 10/1016 UTC from Region 9302 (N19, L = 088, class/area Cso/110 on 5 January), which was in a short-lived growth phase at the time of the flare. Region 9306 produced a long-duration C5/1n flare at 10/0103 UTC associated with a partial- halo CME, and Type II and IV radio sweeps. Another Type IV radio sweep occurred at 10/0119 UTC. Activity decreased to low levels during 11 - 14 January due to isolated to occasional low-level C-class subflares. A large filament erupted from the northwest limb at approximately 14/0430 UTC. A large coronal mass ejection followed the eruption, but it did not appear to be Earth-directed. Data were available from the Advanced Composition Explorer (ACE) spacecraft for most of the period. A weak, positive-polarity high speed stream occurred during 10 - 11 January with velocities briefly reaching as high as 510 km/sec during 11 January. A weak shock passed the spacecraft at approximately 13/0200 UTC, presumably associated with the partial-halo CME observed on 10 January. There were no proton events detected at geosynchronous orbit. The greater than 2 MeV electron flux at geosynchronous orbit was at normal levels. Geomagnetic field activity was at quiet to unsettled levels during most of the period. However, an active period occurred during 12/0300 - 0600 UTC. Forecast of Solar and Geomagnetic Activity 17 January - 12 February 2001 Solar activity is expected to be at mostly low levels with isolated M-class flares possible sometime during the period. No proton events are expected during the period. The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal to moderate levels. Geomagnetic field activity is expected to be at quiet to unsettled levels, barring an Earth-directed CME. .