Inizio Max Fine Rgn Loc Xray Op 245MHz 10cm Sweep 2144 2153 2158 0386 S07E55 C5.2 1f 140 2227 2255 2312 0386 M6.8 1200 2100 II/IV
10 cm 122 SSN 080 Afr/Ap 040/050 X-ray Background B2.8 Fluenza di Protoni Giornaliera (accumulo di flusso nelle 24 ore) GT 1 MeV 7.9e+05 GT 10 MeV 1.8e+04 p/(cm2-ster-day) (GOES-8 satellite ad orbita sincrona W127 gradi) Flusso Giornaliero di Elettroni GT 2 MeV 8.00e+06 e/(cm2-ster-day) (GOES-12 satellite ad orbita sincrona W76 gradi) Indice K a 3 ore Boulder 5 5 6 5 4 4 3 4 Planetary 5 6 6 6 4 4 4 4
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.
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