:Product: Weekly Highlights and Forecasts :Issued: 1999 Nov 16 2112 UT HIGHLIGHTS OF SOLAR AND GEOMAGNETIC ACTIVITY 08 - 14 NOVEMBER 1999 SOLAR ACTIVITY WAS MODERATE DURING MOST OF THE PERIOD, BUT INCREASED TO HIGH LEVELS ON 14 NOVEMBER. ACTIVITY ROSE TO HIGH LEVELS ON 14 NOVEMBER DUE TO A PAIR OF MAJOR FLARES. THE FIRST WAS AN M8/2B AT 14/1801UT FROM REGION 8763 (S14, L=249, CLASS/AREA DAO/170 ON 11 NOVEMBER). THE SECOND WAS AN M5/2N AT 14/1607UT FROM REGION 8766 (N18, L=210, CLASS/AREA DAO/190 ON 14 NOVEMBER). BOTH FLARES WERE IMPULSIVE AND WERE ASSOCIATED WITH RELATIVELY MINOR DISCRETE RADIO EMISSION. THERE WERE SEVERAL REGIONS ON THE DISK (INCLUDING THOSE MENTIONED ABOVE) THAT PRODUCED ISOLATED M-CLASS SUBFLARES DURING THE PERIOD (SEE THE ENERGETIC EVENT SUMMARY FOR EVENT TIMES). ALL OF THESE REGIONS EXHIBITED MIXED-POLARITY MAGNETIC STRUCTURES OF VARYING COMPLEXITY. REGIONS 8759 (N10, L=287, CLASS/AREA FKC/920 ON 09 NOVEMBER), 8765 (S12, L=235, CLASS/AREA EKC/640 ON 14 NOVEMBER, AND 8766 (N18, L=210, CLASS/AREA DAO/190 ON 14 NOVEMBER) ALSO CONTAINED MAGNETIC DELTA CONFIGURATIONS. REAL-TIME SOLAR WIND DATA WERE AVAILABLE FROM THE ADVANCED COMPOSITION EXPLORER (ACE) SPACECRAFT FOR MOST OF THE PERIOD. CORONAL HOLE EFFECTS WERE OBSERVED DURING 08 - 11 NOVEMBER WITH VELOCITIES PEAKING AT 760 KM/SEC AND IMF BZ RANGING FROM PLUS 09 NT (GSM) TO MINUS 08 NT. CORONAL HOLE EFFECTS SUBSIDED ON 12 NOVEMBER. A CHANGE IN WIND FLOW CHARACTERISTICS OCCURRED AROUND 12/1600UT FOLLOWED BY INCREASED SOUTHWARD IMF BZ (MAXIMUM SOUTHERLY DEFLECTIONS TO MINUS 12 NT), HIGHLY VARIABLE SOLAR SECTOR ORIENTATION, AND MINOR VELOCITY INCREASES. NO PROTON EVENTS WERE DETECTED AT GEOSYNCHRONOUS ORBIT DURING THE PERIOD. THE GREATER THAN 2 MEV ELECTRON FLUX WAS AT MODERATE TO HIGH LEVELS DURING 09 - 13 NOVEMBER. OTHERWISE, FLUXES WERE AT NORMAL TO MODERATE LEVELS. THE GEOMAGNETIC FIELD WAS DISTURBED DURING 08 - 11 NOVEMBER DUE TO CORONAL HOLE EFFECTS WITH ACTIVE TO MINOR STORM LEVELS DETECTED AT MIDDLE LATITUDES AND ACTIVE TO MAJOR STORM LEVELS AT HIGH LATITUDES. THE WERE ALSO LOCALIZED SEVERE STORM PERIODS AT HIGH LATITUDES DURING THE DISTURBANCE. ACTIVITY DECREASED TO QUIET TO UNSETTLED LEVELS ON 12 NOVEMBER AS CORONAL HOLE EFFECTS SUBSIDED. ANOTHER DISTURBANCE OCCURRED DURING 13 NOVEMBER DUE TO A SUSTAINED PERIOD OF SOUTHWARD IMF BZ (SEE THE SOLAR WIND DISCUSSION ABOVE). ACTIVITY DECREASED TO MOSTLY QUIET TO UNSETTLED LEVELS ON THE FINAL DAY OF THE PERIOD. FORECAST OF SOLAR AND GEOMAGNETIC ACTIVITY 17 NOVEMBER - 13 DECEMBER 1999 SOLAR ACTIVITY IS EXPECTED TO RANGE FROM LOW TO HIGH LEVELS. FREQUENT C-CLASS FLARES ARE LIKELY. ISOLATED M-CLASS FLARES WILL BE POSSIBLE THROUGHOUT THE PERIOD. THERE IS ALSO A GOOD CHANCE FOR ISOLATED MAJOR FLARES THROUGH 25 NOVEMBER, PRINCIPALLY FROM REGIONS 8765 AND 8766. BOTH REGIONS WERE GROWING IN SIZE AND COMPLEXITY AS THE PERIOD ENDED. THERE IS A CHANCE FOR A SOLAR PROTON EVENT AT GEOSYNCHRONOUS ORBIT THROUGH 25 NOVEMBER DUE TO THE MAJOR FLARE POTENTIAL IN REGIONS 8765 AND 8766. REGION 8759 ALSO PROVIDES A SLIGHT CHANCE FOR A PROTON EVENT. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ALTITUDE IS EXPECTED TO BE AT MODERATE TO HIGH LEVELS DURING 05 - 10 DECEMBER WITH NORMAL TO MODERATE LEVELS DURING THE REMAINDER OF THE PERIOD. THE GEOMAGNETIC FIELD IS EXPECTED TO BE AT UNSETTLED TO MINOR STORM LEVELS DURING 04 - 08 DECEMBER DUE TO RECURRENT CORONAL HOLE EFFECTS. OTHERWISE, ACTIVITY IS EXPECTED TO VARY BETWEEN QUIET AND UNSETTLED LEVELS (BARRING ANY EARTH-DIRECTED CORONAL MASS EJECTIONS). .