:Product: Weekly Highlights and Forecasts :Issued: 2000 May 30 2112 UT HIGHLIGHTS OF SOLAR AND GEOMAGNETIC ACTIVITY 22 - 28 MAY 2000 SOLAR ACTIVITY WAS AT LOW TO MODERATE LEVELS. LOW ACTIVITY PREVAILED MOST OF THE PERIOD, BUT ROSE TO MODERATE LEVELS ON 24 MAY DUE TO AN M1/SF FLARE AT 24/0546UT FROM REGION 8996 (S21, L = 345, CLASS/AREA EKC/1280 ON 15 MAY) AND AN OPTICALLY UNCORRELATED M1 AT 24/1152UT. REGION 8996 WAS GRADUALLY DECAYING AT THE TIME OF THE FLARE. OCCASIONAL C-CLASS SUBFLARES OCCURRED DURING THE REST OF THE PERIOD REAL-TIME SOLAR WIND DATA WERE AVAILABLE FROM THE NASA ADVANCED COMPOSITION EXPLORER (ACE) SPACECRAFT FOR MOST OF THE PERIOD. A CORONAL MASS EJECTION (CME) SIGNATURE WAS OBSERVED DURING 23 - 25 MAY. THE CME SHOCK FRONT PASSED THE ACE SPACECRAFT AT 23/1625UT FOLLOWED BY INCREASED VELOCITIES, DENSITIES, AND IMF BZ VARIABILITY. EARLY ON 24 MAY VELOCITIES PEAKED AT 730 KM/SEC AND DENSITIES PEAKED AT 51 P/CC, FOLLOWED BY A GRADUAL DECLINE. IMF BZ BECAME STRONGLY SOUTHWARD EARLY ON 24 MAY WITH MAXIMUM DEFLECTIONS TO MINUS 36 NT (GSM). BZ REMAINED MOSTLY SOUTHWARD THROUGH MIDDAY ON 26 MAY WITH A RANGE OF MINUS 01 TO 05 NT. NOMINAL SOLAR WIND CONDITIONS WERE OBSERVED BEGINNING MIDDAY ON 26 MAY. THERE WERE NO PROTON EVENTS DETECTED AT GEOSYNCHRONOUS ORBIT. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT INCREASED TO MODERATE TO HIGH LEVELS DURING 25 - 28 MAY. GEOMAGNETIC STORM CONDITIONS WERE OBSERVED DURING 23 - 26 MAY DUE TO A CME PASSAGE AT EARTH. THE STORM BEGAN LATE ON 23 MAY, THEN INTENSIFIED EARLY ON 24 MAY WITH MINOR TO SEVERE STORM LEVELS DETECTED AT ALL LATITUDES. THE SEVERE STORM LEVELS OCCURRED DURING 24/0000 - 0600UT. MINOR TO MAJOR STORM PERIODS OCCURRED DURING 25 - 26 MAY AS THE DISTURBANCE GRADUALLY SUBSIDED. FIELD ACTIVITY DECLINED TO MOSTLY QUIET TO UNSETTLED LEVELS AFTER 26/1200UT. THE SOURCE FOR THIS DISTURBANCE MAY HAVE BEEN A LONG-DURATION C7/1N FLARE AT 20/0535UT WITH AN ASSOCIATED PARTIAL-HALO CME. FORECAST OF SOLAR AND GEOMAGNETIC ACTIVITY 31 MAY - 26 JUNE 2000 SOLAR ACTIVITY IS EXPECTED TO VARY BETWEEN LOW AND MODERATE LEVELS. ISOLATED M-CLASS FLARES WILL BE MOST LIKELY DURING 07 - 23 JUNE. NO PROTON EVENTS ARE EXPECTED AT GEOSYNCHRONOUS ORBIT. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT IS EXPECTED TO BE AT MODERATE TO HIGH LEVELS THROUGH 02 JUNE. NORMAL TO MODERATE LEVELS ARE EXPECTED FOR THE REST OF THE PERIOD. ACTIVE PERIODS ARE EXPECTED DURING 31 MAY, 12 - 13 JUNE AND 25 - 26 JUNE DUE TO CORONAL HOLE EFFECTS. QUIET TO UNSETTLED LEVELS ARE EXPECTED DURING THE REMAINDER OF THE PERIOD, BARRING AN EARTH-DIRECTED CME. .