Viendo archivo del domingo, 18 mayo 2003
Informe geofísico
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.
Resumen de Actividad Solar y Geofísica 2003 May 18 0245 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.comResumen conjunto USAF/NOAA actividad Solar y Geofísica
SGAS Número 138 publicado el 0245Z a las 18 May 2003
Este infórmese ha elaborado a partir de los datos recibidos en SWO el 17 May
A. Eventos Energéticos
Inicio Max Fin Rgn Loc Xray Op 245MHz 10cm Barrido
0305 0306 0306 110
B. Eventos de Protones
Ninguno.
C. Resumen de Actividad Geomagnética
The geomagnetic field has been at
quiet to unsettled levels. The greater than 2 MeV electron flux at
geosynchronous orbit reached high levels today.
D. Estratosfera caliente
Ninguno.
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 102 SSN 081 Afr/Ap 010/009 X-ray Background B1.6
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV 1.6e+05 GT 10 MeV 1.1e+04 p/(cm2-ster-day)
(Satélite órbita sincronizada GOES-8 , W93 grados)
Fluidez diaria de electrones
GT 2 MeV 2.70e+08 e/(cm2-ster-day)
(Satélite órbita sincronizada GOES-12 , W75 grados)
3 Horas K-índices
Boulder 2 3 3 2 3 3 1 2 Planetary 3 3 3 2 3 2 1 ?
F. Comentarios
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. As of 1500 UT on May 15, GOES-8 became 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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