:Product: Weekly Highlights and Forecasts :Issued: 2000 Mar 21 2112 UT HIGHLIGHTS OF SOLAR AND GEOMAGNETIC ACTIVITY 13 - 19 MARCH 2000 SOLAR ACTIVITY WAS PREDOMINANTLY MODERATE FOR THE WEEK. A TOTAL OF 7 LOW-LEVEL M-CLASS EVENTS WAS OBSERVED. REGION 8906 (S16, L=122, CLASS AREA EKC/900 ON 14 MARCH) WAS RESPONSIBLE FOR 6 OF THOSE M-CLASS FLARES. THIS REGION EXHIBITED SIGNIFICANT MAGNETIC COMPLEXITY, INCLUDING SEVERAL DELTA CONFIGURATIONS, DURING THE PERIOD. REGION 8910 (N12, L=071, CLASS/AREA EKC/590 ON 19 MARCH) WAS RESPONSIBLE FOR THE OTHER M-CLASS EVENT. THIS REGION GREW AT A MODERATE PACE DURING THE PERIOD AND DEVELOPED A DELTA CONFIGURATION AT THE END OF THE PERIOD. MANY CORONAL MASS EJECTIONS OCCURRED DURING THE WEEK. NONE APPEARED TO BE EARTH DIRECTED. REAL-TIME SOLAR WIND DATA WERE AVAILABLE FROM THE NASA ADVANCED COMPOSITION EXPLORER (ACE) SPACECRAFT FOR ALMOST ALL OF THE PERIOD. SOLAR WIND VELOCITY WAS BELOW NORMAL FOR MOST OF THE TIME AND OTHER PARAMETERS WERE NOMINAL. THERE WERE NO PROTON EVENTS DETECTED AT GEOSYNCHRONOUS ORBIT. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT WAS AT NORMAL TO MODERATE LEVELS. THE GEOMAGNETIC FIELD WAS GENERALLY QUIET FOR THE WEEK. BRIEF UNSETTLED CONDITIONS WERE OBSERVED TOWARD THE END OF THE PERIOD. FORECAST OF SOLAR AND GEOMAGNETIC ACTIVITY 22 MARCH - 17 APRIL 2000 SOLAR ACTIVITY SHOULD BE GENERALLY MODERATE FOR THE NEXT 27 DAYS. REGION 8910 IS CAPABLE OF GENERATING OCCASIONAL M-CLASS FLARES PRIOR TO ITS WEST LIMB TRANSIT ON 25-26 MARCH. THERE IS A SLIGHT POSSIBILITY OF A MAJOR FLARE FROM THIS REGION PRIOR TO THAT TIME. PREVIOUSLY ACTIVE LONGITUDES ARE EXPECTED TO RETURN DURING THE NEXT TWO WEEKS THAT SHOULD HELP MAINTAIN MODERATE LEVELS OF ACTIVITY FOR THE FORESEEABLE FUTURE. SHOULD REGION 8910 PRODUCE A MAJOR FLARE, THERE IS A POSSIBILITY OF A SOLAR PROTON EVENT DURING THE EARLY PART OF THE FORECAST PERIOD. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT SHOULD BECOME ELEVATED DURING THE 25-28 MARCH PERIOD. NORMAL LEVELS ARE FORECAST FOR THE REMAINDER OF THE UPCOMING SOLAR ROTATION. THE GEOMAGNETIC FIELD SHOULD REMAIN QUIET TO UNSETTLED UNTIL 24 MARCH WHEN A CORONAL HOLE RELATED DISTURBANCE IS EXPECTED TO BEGIN. PREDOMINANTLY UNSETTLED TO ACTIVE CONDITIONS SHOULD BE EXPERIENCED THROUGH 26 MARCH. ISOLATED MINOR STORM CONDITIONS ARE POSSIBLE DURING THAT PERIOD. BARRING THE OCCURRENCE OF FUTURE EARTH DIRECTED CORONAL MASS EJECTIONS, THE REMAINDER OF THE PERIOD SHOULD CONSIST OF QUIET TO UNSETTLED CONDITIONS. .