Viendo archivo del sábado, 19 enero 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 Jan 19 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 019 Publicado el 2200Z a las 19 Jan 2002

IA. Análisis de regiones solares activas y de actividad desde 18-2100Z hasta 19-2100Z

Solar activity increased to moderate levels. Region 9787 (S07E59) produced an impulsive M1/Sf flare at 19/1005 UTC with minor radio emission. Minor growth occurred in this region, but it remained simply structured. Minor growth also occurred in Regions 9786 (S25W32) and 9788 (N17E40), but both remained simple bipoles. Region 9788 produced a low-level C-class flare late in the period. Region 9782 showed a minor decrease in area and continued to display minor polarity mixing within its southern leader spots. A large filament disappeared from the northeast quadrant late on 18 January. SOHO EIT/LASCO images showed that the filament gradually disappeared and was followed by a relatively slow, non-Earth directed CME. New Regions 9789 (N15W02) and 9790 (N28E25) were numbered.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low to moderate. There will be a chance for an isolated low-level M-class flare during the period.
IIA. Resumen de la actividad geofísica 18-2100Z a 19-2100Z
Geomagnetic field activity ranged from quiet to minor storm levels. Activity increased to unsettled to minor storm levels during 19/1200 - 1800 UTC, then decreased to mostly unsettled levels. The increased activity was likely due to coronal hole effects.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is expected to be at quiet to unsettled levels during most of the period. However, brief active conditions will be possible early in the period due to coronal hole effects.
III. Probabilidades del evento 20 Jan a 22 Jan
Clase M40%40%40%
Clase X05%05%05%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       19 Jan 214
  Previsto   20 Jan-22 Jan  220/225/230
  Media de 90 Días        19 Jan 223
V. Índices Geomagnéticos A
  Observado Afr/Ap 18 Jan  005/005
  Estimado     Afr/Ap 19 Jan  012/012
  Previsto    Afr/Ap 20 Jan-22 Jan  012/010-010/010-008/008
VI. Probabilidades de Actividad Geomagnética 20 Jan a 22 Jan
A. Latitudes Medias
Activo35%30%20%
Tormenta Menor10%05%01%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo45%35%25%
Tormenta Menor15%10%05%
Tormenta Mayor-Severa05%05%01%

All times in UTC

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