Viendo archivo del sábado, 1 noviembre 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 Nov 01 0245 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Resumen conjunto USAF/NOAA actividad Solar y Geofísica

SGAS Número 305 publicado el 0245Z a las 01 Nov 2003 Este infórmese ha elaborado a partir de los datos recibidos en SWO el 31 Oct
A. Eventos Energéticos
Inicio  Max  Fin  Rgn   Loc   Xray  Op 245MHz 10cm   Barrido
0353 0353 0353                       300
0426 0433 0437              M2.0            67
0552 0553 0553                       590
0608 0616 0628  0488 N08W28 M1.1  Sf
1121 1122 1125                       200    140
1141 1142 1142                       240
1507 1507 1508                       120
1644 1706 1748  0486 S20W28 C5.3  Sf 220    37
1844 1844 1845                       730
2006 2006 2007                       1000
B. Eventos de Protones
The greater than 100 MeV proton event in progress since 28/1145Z, ended at 31/0145Z. This prolonged high energy proton event was actually two distinct events associated with the X17 and X10 flares on the 28th and 29th respectively. The peak measurements for both events were 186 pfu at 29/0015Z and 110 pfu at 29/2310Z. The greater than 10 MeV proton event remains in progress, but is quickly declining to the 10 pfu alert threshold. The two peak measurements at 10 MeV were 29,000 pfu at 29/0615Z and 3300 pfu at 30/1935Z. The PCA event has ended.
C. Resumen de Actividad Geomagnética
The geomagnetic field ranged from active to severe storm levels. The intense geomagnetic storm that began at around 30/1600Z, continued into the early stages of this period. Severe storm levels persisted from 31/0000Z through 31/0900Z. Mostly active to major storm periods occurred through the latter half of the period. Solar radiation contamination on the ACE SWEPAM instrument finally ended at 31/0052Z. Solar wind speed was at an exceptionally high 1200 km/s, but has been in a gradual decline, ending the period at over 800 km/s. The prolonged periods of southward IMF Bz that occurred early in the period have ended. Bz has been mostly northward since 31/0200Z.
D. Estratosfera caliente
Ninguno
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 249  SSN 266  Afr/Ap 065/093   X-ray Background C1.8
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV 9.8e+07   GT 10 MeV 7.0e+06 p/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-11 , W107 grados)
Fluidez diaria de electrones
GT 2 MeV 3.40e+06 e/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-12 , W75 grados)
3 Horas K-índices
Boulder 7 6 7 5 5 4 3 4 Planetary 8 7 7 6 6 5 4 4
F. Comentarios
  Ninguno

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