Inizio Max Fine Rgn Loc Xray Op 245MHz 10cm Sweep 2227 2255 2312 0386 M6.8 1200 2100 II/IV
10 cm 120 SSN 099 Afr/Ap 045/054 X-ray Background B3.2 Fluenza Protonica Giornaliera (accumulo di flusso in 24 ore) GT 1 MeV 2.5e+07 GT 10 MeV 1.4e+06 p/(cm2-ster-day) (Orbita sincrona di W128 gradi del satellite GOES-8) Fluenza di Elettroni Giornaliera GT 2 MeV 2.30e+06 e/(cm2-ster-day) (Orbita sincrona di W75 gradi del satellite GOES-12) Indice K di 3 ore Boulder 5 5 6 6 3 5 4 3 Planetary 5 6 7 6 4 4 4 4
Nessuna PLAIN K-Indices: On 16 June, it was determined that a scaling problem exists with 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. GOES 11 (113W) will become the primary satellite for protons. The transition from GOES 8 to GOES 11 was scheduled for 18 June, but has been delayed until 19 June. 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. 99999
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