Viendo archivo del sábado, 5 octubre 2002

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 2002 Oct 05 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 278 Publicado el 2200Z a las 05 Oct 2002

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

Solar activity reached high levels again this period. Region 139 (N12E32) produced a major flare late in the period, an M5/1n flare (in progress at issue time), and a Type II radio sweep (404 km/s). The flare began at 05/2042Z and appears to have peaked at M5.9 at 2100Z. This region also produced an M2/Sf at 04/2243Z with associated Type II sweep (418 km/s). The rapid growth observed yesterday has slowed considerably, and though no delta configuration is obvious today, the region continues to grow slowly and now nears 700 millionths of white light areal coverage. Region 137 (S19W33) produced an M1/Sf at 05/1046Z. This region has settled down after producing four M-class flares in the last period. Some slight decay was noted. New Regions 141 (S07E20) and 142 (N07E64) were numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to continue at moderate to high levels. M-class activity is likely from Regions 137 and 139, and there's a small chance for another major flare from Region 139.
IIA. Resumen de la actividad geofísica 04-2100Z a 05-2100Z
The geomagnetic field was at unsettled to minor storm levels. The Bz component of the interplanetary magnetic field continues to be predominantly southward. The greater than 2 MeV electron flux reached moderate to high levels.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to continue at unsettled to minor storm levels. Transient effects from the rather weak CMEs on 3 and 4 Oct may enhance the disturbed periods on days one and two. A large, recurrent southern coronal hole will move into geoeffective position late on day two through day three.
III. Probabilidades del evento 06 Oct a 08 Oct
Clase M60%50%50%
Clase X10%10%10%
Protón05%05%05%
PCAFyellow
IV. Penticton 10.7cm flujo
  Observado       05 Oct 155
  Previsto   06 Oct-08 Oct  160/170/175
  Media de 90 Días        05 Oct 179
V. Índices Geomagnéticos A
  Observado Afr/Ap 04 Oct  043/048
  Estimado     Afr/Ap 05 Oct  022/025
  Previsto    Afr/Ap 06 Oct-08 Oct  020/020-020/020-025/025
VI. Probabilidades de Actividad Geomagnética 06 Oct a 08 Oct
A. Latitudes Medias
Activo50%50%50%
Tormenta Menor25%25%25%
Tormenta Mayor-Severa10%10%10%
B. Latitudes Altas
Activo50%50%50%
Tormenta Menor35%35%35%
Tormenta Mayor-Severa15%10%10%

All times in UTC

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