Viewing archive of söndag, 22 juni 2003
Geofysisk rapport
Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Sammanfattning av sol- och geofysisk aktivitet 2003 Jun 22 0245 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.comUSAF/NOAAs sammanfattning av sol- och geofysisk aktivitet
SGAS nummer 173 publicerat klockan 0245Z på 22 Jun 2003
Den här rapporten har sammanställts med data från SWO på 21 Jun
A. Energihöga händelser
Start Max Ände Region Plats Xray På 245MHz 10 cm Sweep
0009 0014 0018 0386 C1.7 260
0023 0024 0027 330
0145 0145 0145 150
0317 0317 0319 110
B. Protonstormar
Ingen
C. Sammanfattning av geofysisk aktivitet
The geomagnetic field was at
unsettled to minor storm levels. Sustained periods of southward Bz
along with elevated solar wind speeds led to the occasional storming
conditions. The greater than 2 MeV electron flux at geosynchronous
orbit reached high levels today.
D. Stratwarm
Ingen
E. Dagligt index (uppskattade/förväntade värden i realtid)
10 cm 115 SSN 118 Afr/Ap 026/023 X-ray Background MSG
Daglig protonenergi (flux-ackumulering över 24 timmar)
GT 1 MeV MSG GT 10 MeV MSG p/(cm2-ster-day)
(GOES-11 satellit synkron rotation W113 grader)
Daglig elektronenergi
GT 2 MeV MSG e/(cm2-ster-day)
(GOES-12 satellit synkron rotation W75 grader)
K-index för 3 timmar
Boulder 4 3 5 3 3 5 4 3 Planetary 4 4 5 3 3 4 3 3
F. Kommentarer
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) is now 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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