Viendo archivo del lunes, 13 abril 2009

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 2009 Apr 13 2201 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 103 Publicado el 2200Z a las 13 Apr 2009

IA. Análisis de regiones solares activas y de actividad desde 12-2100Z hasta 13-2100Z

Solar activity was very low. No flares occurred during the past 24 hours. The solar disk continues to be void of sunspots.
IB. Pronóstico de la actividad solar
Solar activity is expected to be very low.
IIA. Resumen de la actividad geofísica 12-2100Z a 13-2100Z
The geomagnetic field was quiet to unsettled. Solar wind velocity at ACE showed a steady declining trend with day-end values around 380 km/s. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the past 24 hours.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be quiet for the next three days (14-16 April).
III. Probabilidades del evento 14 Apr a 16 Apr
Clase M01%01%01%
Clase X01%01%01%
Protón01%01%01%
PCAFGreen
IV. Penticton 10.7cm flujo
  Observado       13 Apr 068
  Previsto   14 Apr-16 Apr  068/068/068
  Media de 90 Días        13 Apr 070
V. Índices Geomagnéticos A
  Observado Afr/Ap 12 Apr  004/008
  Estimado     Afr/Ap 13 Apr  005/005
  Previsto    Afr/Ap 14 Apr-16 Apr  005/005-005/005-005/005
VI. Probabilidades de Actividad Geomagnética 14 Apr a 16 Apr
A. Latitudes Medias
Activo05%05%05%
Tormenta Menor01%01%01%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo05%05%05%
Tormenta Menor01%01%05%
Tormenta Mayor-Severa01%01%01%

All times in UTC

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