Viendo archivo del viernes, 12 noviembre 2004
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.
:Product: 20041112SGAS.txt
:Issued: 2004 Nov 12 0250 UT
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Resumen conjunto USAF/NOAA actividad Solar y Geofísica
SGAS Número 317 publicado el 0245Z a las 12 Nov 2004
Este infórmese ha elaborado a partir de los datos recibidos en SWO el 11 Nov
A. Eventos Energéticos
Inicio Max Fin Rgn Loc Xray Op 245MHz 10cm Barrido
0441 0441 0441 87 IV
1029 1029 1033 100
1508 1523 1532 0696 B9.0 130
1543 1544 1545 410
1548 1548 1548 130
B. Eventos de Protones
The greater than 10 MeV proton event that began
at 07/1910Z remains in progress (currently ranging from 50 - 100
pfu). The maximum so far was 495 pfu at 08/0115Z.
C. Resumen de Actividad Geomagnética
The geomagnetic field ranged from
quiet to minor storm levels. The most disturbed levels followed a
prolonged period of southward Bz between 11/03 - 07Z. Solar wind
speed was elevated between 550 and 650 km/s. A 12 nT sudden impulse
was observed at the geomagnetic field at 11/1714Z. Solar wind plasma
and magnetic field measurements at ACE indicate weak transient flow,
likely from the CME activity on 09 - 10 November.
D. Estratosfera caliente
Ninguno
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 095 SSN 070 Afr/Ap 022/023 X-ray Background B2.1
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV 1.1e+08 GT 10 MeV 6.9e+06 p/(cm2-ster-day)
(Satélite órbita sincronizada GOES-11 , W102 grados)
Fluidez diaria de electrones
GT 2 MeV 1.40e+09 e/(cm2-ster-day)
(Satélite órbita sincronizada GOES-12 , W75 grados)
3 Horas K-índices
Roca 4 5 3 4 2 3 3 4 Planetario 4 5 4 4 2 3 2 4
F. Comentarios
The greater than 2 MeV electron fluence at
geosynchronous orbit was at very high levels.
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