:Product: Report of Solar-Geophysical Activity :Issued: 2010 May 11 2201 UTC # Prepared jointly by the U.S. Dept. of Commerce, NOAA, # Space Weather Prediction Center and the U.S. Air Force. # Joint USAF/NOAA Report of Solar and Geophysical Activity SDF Number 131 Issued at 2200Z on 11 May 2010 IA. Analysis of Solar Active Regions and Activity from 10/2100Z to 11/2100Z: Solar activity was very low. The visible disk remained spotless. IB. Solar Activity Forecast: Solar activity is expected to remain at very low levels. IIA. Geophysical Activity Summary 10/2100Z to 11/2100Z: The geomagnetic field was at quiet to unsettled levels. A solar sector boundary crossing from negative (toward) to positive (away) was evident in ACE SWEPAM signatures at about 11/0130Z. Shortly afterwards, solar wind velocity gradually increased from about 350 km/s to near 400 km/s by 0600Z, while the Bz component of the interplanetary magnetic field turned southward (-5 nT). These signatures were consistent with a co-rotating interaction region in advance of a coronal hole high speed wind stream. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels. IIB. Geophysical Activity Forecast: The geomagetic field is expected to be at quiet to unsettled levels, with isolated active periods, all three days of the forecast period (12 - 14 May). This activity is due to a series of coronal hole high speed wind streams that are located in both solar hemispheres. III. Event Probabilities 12 May-14 May Class M 01/01/01 Class X 01/01/01 Proton 01/01/01 PCAF green IV. Penticton 10.7 cm Flux Observed 11 May 074 Predicted 12 May-14 May 074/073/073 90 Day Mean 11 May 081 V. Geomagnetic A Indices Observed Afr/Ap 10 May 004/005 Estimated Afr/Ap 11 May 008/008 Predicted Afr/Ap 12 May-14 May 010/010-008/008-008/008 VI. Geomagnetic Activity Probabilities 12 May-14 May A. Middle Latitudes Active 30/25/25 Minor storm 10/05/05 Major-severe storm 01/01/01 B. High Latitudes Active 35/30/30 Minor storm 15/10/10 Major-severe storm 01/01/01