Viewing archive of tisdag, 24 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 24 0245 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com

USAF/NOAAs sammanfattning av sol- och geofysisk aktivitet

SGAS nummer 175 publicerat klockan 0245Z på 24 Jun 2003 Den här rapporten har sammanställts med data från SWO på 23 Jun
A. Energihöga händelser
Start  Max  Ände Region Plats   Xray  På 245MHz 10 cm   Sweep
1653 1653 1653                       1400
B. Protonstormar
Ingen
C. Sammanfattning av geofysisk aktivitet
The geomagnetic field was unsettled to active with an isolated minor storm period between 23/03-06Z. The field was disturbed due to a high speed coronal hole stream which peaked near 600 km/s very early in the period.
D. Stratwarm
Ingen
E. Dagligt index (uppskattade/förväntade värden i realtid)
10 cm 114  SSN 104  Afr/Ap 022/020   X-ray Background B1.9
Daglig protonenergi (flux-ackumulering över 24 timmar)
GT 1 MeV 3.1e+06   GT 10 MeV 1.2e+04 p/(cm2-ster-day)
(GOES-11 satellit synkron rotation W113 grader)
Daglig elektronenergi
GT 2 MeV 1.40e+08 e/(cm2-ster-day)
(GOES-12 satellit synkron rotation W75 grader)
K-index för 3 timmar
Boulder 3 5 4 4 3 3 3 3 Planetary 4 5 4 4 3 3 3 3
F. Kommentarer
The scaling problem with the Boulder magnetometer instrument has been fixed and the instrument has been redesignated as the primary instrument for Boulder K-indices.

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.

The problem with missing particle fluence data and X-ray background value has been corrected. Those missing values can now be found at:
http://www.sec.noaa.gov/ftpdir/indices/DPD.txt
http://www.sec.noaa.gov/ftpdir/latest/DSD.txt

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