:Product: 04231230forecast_discussion.txt :Issued: 2014 Apr 23 1230 UTC # Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center # Solar Activity .24 hr Summary... Solar activity was at low levels due to only four C-class flares occurring during the past 24 hours. Region 2038 (S11W40, Dai/beta-gamma) was responsible for half of the flare activity, including the largest flare of the period, a C4/Sf flare at 23/0104 UTC. Region 2035 (S13W78, Ekc/beta-gamma) remained one of the most magnetically complex regions on the visible disk, yet was fairly inactive. The remaining spotted regions were either relatively stable or showed slight decay. No new regions were numbered. No Earth-directed coronal mass ejections (CMEs) were observed during the period. .Forecast... Solar activity is expected to be at low levels, with a chance for M-class flares (NOAA Scale R1/R2 - Minor/Moderate) for the forecast period (23-25 Apr) as Regions 2034, 2035, and 2036 make their way around the west limb. Energetic Particle .24 hr Summary... The greater than 2 MeV electron flux at geosynchronous orbit was at normal levels. The greater than 10 MeV proton flux was at background levels. .Forecast... The greater than 2 MeV electron flux at geosynchronous orbit is expected to be at normal to moderate levels for the forecast period. The greater than 10 MeV proton flux at geosynchronous orbit is also expected remain at nominal levels for the forecast period (23-25 Apr). Solar Wind .24 hr Summary... Solar wind parameters, measured at the ACE spacecraft, continued to show signs of nominal conditions. Bt remained steady between 2 nT and 4 nT, and solar wind speeds decreased from around 470 km/s to near 430 km/s. Bz held steady between +/- 2nT until just after 23/0300 UTC, when it began varying between +/-4 nT. Phi angle remained in a mostly positive (away) orientation until just before the start of the new UTC day. Shortly after 23/2235 UTC, Phi angle oscillated to a negative (towards) orientation, where it remained through the end of the period. .Forecast... A negative polarity solar wind feature is still expected mid-day on day one (23 Apr) based on recurrence, and should persist through days two and three (24-25 Apr). Wind speeds near 550 km/s are expected with intermittent southward Bz as well. Geospace .24 hr Summary... The geomagnetic field was quiet. .Forecast... Quiet to unsettled conditions are expected for the next three days (23-25 Apr), due to a weak recurrent negative polarity feature in the solar wind stream.