:Product: 20030617RSGA.txt :Issued: 2003 Jun 17 2200 UTC # Prepared jointly by the U.S. Dept. of Commerce, NOAA, # Space Environment Center and the U.S. Air Force. # Joint USAF/NOAA Report of Solar and Geophysical Activity SDF Number 168 Issued at 2200Z on 17 Jun 2003 IA. Analysis of Solar Active Regions and Activity from 16/2100Z to 17/2100Z: Solar activity was at low levels. The largest flare was a C2 flare at 0222 UTC from Region 386 (S07E58). This region continues to increase in area coverage as it rotates further onto the visible disk. Magnetic analysis indicates a beta-gamma magnetic configuration. Region 380 (S15W64) continues a its gradual decay in area and now has a beta magnetic configuration. IB. Solar Activity Forecast: Solar activity is expected to be at low to moderate levels with a chance of isolated high level activity. Region 386 has the potential for major flare activity. IIA. Geophysical Activity Summary 16/2100Z to 17/2100Z: The geomagnetic field was at active to major storm levels. A six-hour period of southward Bz, from 06 - 09 UTC combined with elevated solar wind speed near 510 km/s produced minor and major storm levels. IIB. Geophysical Activity Forecast: The geomagnetic field is expected to be at unsettled to minor storm levels. A weak CME shock is possible late on day one with isolated minor storm levels possible. High speed stream effects are expected on day two and day three with minor storm levels possible. III. Event Probabilities 18 Jun-20 Jun Class M 40/40/40 Class X 20/20/20 Proton 30/20/20 PCAF green IV. Penticton 10.7 cm Flux Observed 17 Jun 122 Predicted 18 Jun-20 Jun 125/120/120 90 Day Mean 17 Jun 125 V. Geomagnetic A Indices Observed Afr/Ap 16 Jun 020/032 Estimated Afr/Ap 17 Jun 040/050 Predicted Afr/Ap 18 Jun-20 Jun 020/030-020/030-020/025 VI. Geomagnetic Activity Probabilities 18 Jun-20 Jun A. Middle Latitudes Active 35/40/40 Minor storm 15/20/20 Major-severe storm 05/05/05 B. High Latitudes Active 40/50/50 Minor storm 20/25/25 Major-severe storm 10/15/15 VII Comment: K-Indices: On 16 June, it was determined that a scaling problem exists with the H-trace on the Boulder magnetometer instrument. While this problem, and its fix are being investigated the primary instrument for Boulder K-indices has been switched to the Boulder USGS (via Domsat) magnetometer, effective 1500 UTC on 16 June. GOES Protons: To ensure continued operational monitoring of important energetic particle data, it is necessary to reassign primary/secondary designations for the GOES Space Environment Monitor (SEM) detectors. Beginning 1700 UTC on June 18, GOES 11 (105W) will become the primary satellite for protons. GOES 12 will continue as the primary satellite for magnetometer, X-ray, and electron measurements. GOES 10 (135W) will be the secondary satellite for all SEM sensors - magnetometer, X-ray, and energetic particles. Because of the degraded state of the proton data on GOES-10, its designation as the secondary source for proton data is a short-term solution. More permanent solutions have been identified and are being evaluated. Users will be notified when we define and schedule a permanent fix. Further details can be found at http://www.sec.noaa.gov/GOES.html.