Viewing archive of torsdag, 15 maj 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 May 15 0245 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com

USAF/NOAAs sammanfattning av sol- och geofysisk aktivitet

SGAS nummer 135 publicerat klockan 0245Z på 15 May 2003 Den här rapporten har sammanställts med data från SWO på 14 May
A. Energihöga händelser
Start  Max  Ände Region Plats   Xray  På 245MHz 10 cm   Sweep
Ingen
B. Protonstormar
Ingen.
C. Sammanfattning av geofysisk aktivitet
The geomagnetic field has been at unsettled to minor storm levels due to a favorably positioned coronal hole. 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 096  SSN 075  Afr/Ap 025/027   X-ray Background B1.0
Daglig protonenergi (flux-ackumulering över 24 timmar)
GT 1 MeV 6.8e+06   GT 10 MeV 1.1e+04 p/(cm2-ster-day)
(GOES-10 satellit synkron rotation W135 grader)
Daglig elektronenergi
GT 2 MeV 7.80e+08 e/(cm2-ster-day)
(GOES-10 satellit synkron rotation W135 grader)
K-index för 3 timmar
Boulder 5 5 5 4 3 3 4 3 Planetary 5 5 5 4 3 4 4 3
F. Kommentarer
  The GOES 10 energetic proton detectors are showing
intermittent, high noise levels in the higher energy proton channels
(greater than about 80 MeV). This problem was first noticed in data
taken April 26, 2003. 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 1500 UT on May 15, GOES-8 will
once again become the primary satellite for protons. GOES 12 will be
the primary satellite for magnetometer, X-ray, and electron
measurements. GOES 10 will be the secondary satellite for all SEM
sensors - magnetometer, X-ray sensor, and energetic particle sensor.
This short-term solution (approximately 2 - 3 months) will be in
place until we define and implement a permanent fix. A more detailed
explanation can be found at: http://www.sec.noaa.gov/GOES.html.

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