Viendo archivo del viernes, 5 noviembre 2004

Informe actividad solar

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.
Informe de actividad Solar-Geofísica 2004 Nov 05 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 310 Publicado el 2200Z a las 05 Nov 2004

IA. Análisis de regiones solares activas y de actividad desde 04-2100Z hasta 05-2100Z

Solar activity increased to high levels today. Region 696 (N09E06) produced the largest flare of the period, an M5 major flare at 04/2309Z that had an associated Tenflare (1800 sfu's), Type IV spectral radio sweep, and a Type II sweep with an estimated shock velocity of 1053 km/sec. An M2/1n event occurred at 04/2229Z. The combination of these two flares resulted in a complex partial halo CME that should become geoeffective. Region 696 also produced an M4/1f at 05/1130Z that had an associated Tenflare and a Type IV spectral radio sweep and an M1/Sf that occurred at 05/1922Z. This region continues to grow in sunspot area and magnetic complexity while the delta magnetic structure remains well intact. Region 693 (S15W44) has shown steady decay today as the sunspot penumbral converge has lessened and the magnetic delta structure is no longer evident. No new regions were numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at moderate to high levels. Several M-class flares with an isolated major flare are possible from Region 696.
IIA. Resumen de la actividad geofísica 04-2100Z a 05-2100Z
The geomagnetic field was at quiet to unsettled levels today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to range from quiet to major storm levels. The anticipated shock from the full halo CME related to M5/Sn that occurred on 03 November at 1547Z and is expected to arrive on 06 November. A weaker shock is expected late on the sixth, early on 07 November as a result of the long duration C6/Sf event from 04 November that occurred at 0905Z indicated by the resulting partial halo CME. A third shock passage is expected late on the seventh, early on 08 November due to the resulting partial halo CME that occurred today in response to the combination of the M2 and M5 x-ray events of today. Due to the magnetic complexity and frequency of M-class flares from Region 696 there exists a chance for the greater than 10 MeV proton flux at geosynchronous orbit to exceed threshold in response to further major flare activity.
III. Probabilidades del evento 06 Nov a 08 Nov
Clase M75%75%75%
Clase X20%20%20%
Protón20%20%20%
PCAFyellow
IV. Penticton 10.7cm flujo
  Observado       05 Nov 141
  Previsto   06 Nov-08 Nov  140/140/140
  Media de 90 Días        05 Nov 109
V. Índices Geomagnéticos A
  Observado Afr/Ap 04 Nov  005/007
  Estimado     Afr/Ap 05 Nov  005/007
  Previsto    Afr/Ap 06 Nov-08 Nov  025/030-020/020-015/020
VI. Probabilidades de Actividad Geomagnética 06 Nov a 08 Nov
A. Latitudes Medias
Activo40%40%35%
Tormenta Menor35%25%20%
Tormenta Mayor-Severa20%15%10%
B. Latitudes Altas
Activo35%45%45%
Tormenta Menor40%25%25%
Tormenta Mayor-Severa20%15%15%

All times in UTC

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