Viendo archivo del lunes, 23 junio 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 Jun 23 0245 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.comResumen conjunto USAF/NOAA actividad Solar y Geofísica
SGAS Número 174 publicado el 0245Z a las 23 Jun 2003
Este infórmese ha elaborado a partir de los datos recibidos en SWO el 22 Jun
A. Eventos Energéticos
Inicio Max Fin Rgn Loc Xray Op 245MHz 10cm Barrido
0412 0412 0414 910
0536 0540 0544 B6.3 130
0945 0949 0951 0388 N04W28 C1.0 Sf 120
1003 1014 1024 B6.8 150
B. Eventos de Protones
Ninguno
C. Resumen de Actividad Geomagnética
The geomagnetic field was
unsettled to active due to a high speed coronal hole stream.
D. Estratosfera caliente
Ninguno
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 110 SSN 094 Afr/Ap 015/016 X-ray Background Msg
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV Msg GT 10 MeV Msg p/(cm2-ster-day)
(Satélite órbita sincronizada GOES-11 , W113 grados)
Fluidez diaria de electrones
GT 2 MeV Msg e/(cm2-ster-day)
(Satélite órbita sincronizada GOES-12 , W75 grados)
3 Horas K-índices
Boulder 3 3 3 3 3 3 3 3 Planetary 3 3 4 3 3 3 3 3
F. Comentarios
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. The missing (Msg) daily fluence data and the X-ray background data will be corrected on 23 June. Further details can be found at http://www.sec.noaa.gov/GOES.html.
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