Solar Terrestrial Activity Report Last update March 18, 2000 at 04:45 UTC. [Solar and geomagnetic data - last 4 weeks (updated daily)] [Solar wind and electron fluence charts (updated daily)] [Solar cycles 21-23 (last update March 2, 2000)] [Solar cycles 1-20] [Graphical comparison of cycles 21, 22 and 23 (last update March 2, 2000)] [Graphical comparison of cycles 10, 13, 17, 20 and 23 (last update March 2, 2000)] [Historical solar and geomagnetic data charts 1954-1999] Recent development The geomagnetic field was quiet on March 17. Solar wind speed ranged between 306 and 355 km/sec. Solar flare activity was moderate. Solar flux was 192.4, the planetary A index was 6 (3-hour K indices: 2122 2222, Boulder K indices: 1123 2210). Region 8901 was quiet and stable and rotated off the visible disk early today. Region 8906 decayed slowly and will likely continue to produce C flares and occasional minor M flares. There is a chance of a major flare as well. Region 8909 was quiet and stable. Region 8910 developed slowly and has minor M class flaring potential. Region 8911 was quiet and stable and will rotate over the west limb today. Region 8913 developed slowly and could produce further C flares. Region 8914 decayed into spotless plage. Region 8915 was quiet and stable. New region 8916 rotated partly into view at the northeast limb. Further regions will rotate into view over the next couple of days. Flares and CMEs 11 C flares and 1 M flare were recorded on March 17. Region 8906 produced a C5.8 flare at 04:58, a C1.7 flare at 07:20, a C3.3 flare at 07:30, a C1.8 flare at 19:55, a C3.6 flare at 22:00 UTC and an M1.1 flare at 11:25 UTC. Region 8910 generated a C4.3 flare at 08:17 and a C1.8 flare at 09:38 UTC. Region 8913 was the source of a C1.7 flare at 17:17 UTC. A long duration C6 event began before midnight and peaked early on March 18, its source was in region 8906. The background x-ray flux is at the class C1 level. Coronal holes The large coronal hole that has been around for several months has been split into three smaller coronal holes. One is in the northern hemisphere and will rotate into a geoeffective position on March 19, another (and fairly small one) is in the southern hemisphere and could rotate into a geoeffective position on March 20. The third, and largest remaining part, is trans equatorial and should rotate into a geoeffective position on March 21-22. Forecast The geomagnetic field is expected to be quiet to unsettled on March 18-20. A coronal hole related disturbance is likely to start on March 22 and could cause unsettled to active intervals until March 25. Long distance medium wave (AM) band propagation along east-west paths over high and upper middle latitudes is fair. Coronal holes (1)Coronal mass ejections (2)M and X class flares (3) 1) Effects from a coronal hole could reach earth within the next 5 days. 2) Material from a CME is likely to impact earth within 96 hours. 3) There is a possibility of either M or X class flares within the next 48 hours. Green: 0-20% probability, Yellow: 20-60% probability, Red: 60-100% probability. Active solar regions (Recent map) Solar regionDate numberedActual no. sunspotsLocation at midnightAreaClassificationComment 8901200003051S15W860000AXX 890220000306 S17W69 plage 89062000030820S16W490610DKIbeta-gamma 890820000309 S23W31 plage 8909200003113S29E010020CSO 89102000031234N11E050250DAI 8911200003141N08W790010HRX 891220000314 N15W41 plage 89132000031411S16E300100DAO 891420000316 N16W08 plage 8915200003161N23E620130HSX 8916200003171N12E740070HSX Total number of sunspots:72 Monthly solar data MonthAverage solar fluxInternational sunspot numberSmoothed sunspot number 1999.02141.966.184.6 (+2.0) 1999.03126.369.1 83.8 (-0.8) 1999.04117.263.9 85.4 (+1.6) 1999.05148.4106.3 90.4 (+5.0) 1999.06169.8137.7 93.0 (+2.6) 1999.07165.6113.5 94.4 (+1.4) 1999.08170.793.7 97.5 (+3.1) 1999.09135.770.9 (102.6 predicted, +5.1) 1999.10164.8116.4 (107.7 predicted, +5.1) 1999.11191.5132.7 (110.2 predicted, +2.5) 1999.12169.886.4 2000.01158.190.2 2000.02174.1112.3 2000.03204.1 (1)101.8 (2) 1) Running average based on the daily 20:00 UTC solar flux value at 2800 MHz.. 2) Unofficial, accumulated value. The official value is typically 25-40% less. This report has been prepared by Jan Alvestad. It is based partly on my own observations and interpretations, and partly on data from sources in solar links. Comments and suggestions are always welcome. [DX-Listeners' Club] [DX News]