Viewing archive of lördag, 21 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 21 0245 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com

USAF/NOAAs sammanfattning av sol- och geofysisk aktivitet

SGAS nummer 172 publicerat klockan 0245Z på 21 Jun 2003 Den här rapporten har sammanställts med data från SWO på 20 Jun
A. Energihöga händelser
Start  Max  Ände Region Plats   Xray  På 245MHz 10 cm   Sweep
1235 1235 1236                       110
B. Protonstormar
Ingen
C. Sammanfattning av geofysisk aktivitet
The geomagnetic field was at predominantly unsettled levels today as effects from the western most recurrent coronal hole wanes. 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 117  SSN 121  Afr/Ap 014/012   X-ray Background B2
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 3 2 3 3 3 4 3 2 Planetary 3 2 3 3 3 3 3 3
F. Kommentarer
  Ingen
99999
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.
99999

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