Affichage des archives de dimanche, 22 juin 2003
Rapport sur les activités géophysiques
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.
Résumé de l'activité solaire et géophysique 2003 Jun 22 0245 UTC
Fait par le NOAA © SWPC et adapté par SpaceWeatherLive.comRésumé de l'USAF/NOAA sur l'activité solaire et géophysique
SGAS numéro 173 publié à 0245Z le 22 Jun 2003
Ce rapport est une compilation des données reçues à SWO le 21 Jun
A. Evénements énergétiques
Début Max Fin RégionLoc Xray Op 245MHz 10cm Sweep
0009 0014 0018 0386 C1.7 260
0023 0024 0027 330
0145 0145 0145 150
0317 0317 0319 110
B. Tempêtes de protons
Aucun
C. Résumé d'activité géomagnetique
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
Aucun
E. Indices quotidiens (valeurs estimées en temps réel)
10 cm 115 SSN 118 Afr/Ap 026/023 X-ray Background MSG
Fluence journalière de protons (flux protonique par unité d'aire cumulé sur 24h)
GT 1 MeV MSG GT 10 MeV MSG p/(cm2-ster-day)
(Satellite GOES-11 orbite synchrone W113 degrés)
Fluence journalière de protons
GT 2 MeV MSG e/(cm2-ster-day)
(Satellite GOES-12 orbite synchrone W75 degrés)
Indices K sur 24 h (tranches de 3 heures)
Boulder 4 3 5 3 3 5 4 3 Planetary 4 4 5 3 3 4 3 3
F. Commentaires
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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