Viendo archivo del martes, 27 marzo 2007

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 2007 Mar 27 2203 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 086 Publicado el 2200Z a las 27 Mar 2007

IA. Análisis de regiones solares activas y de actividad desde 26-2100Z hasta 27-2100Z

Solar activity was very low. Region 948 (S02W56) has decayed into a unipolar region.
IB. Pronóstico de la actividad solar
Solar activity is expected to be very low.
IIA. Resumen de la actividad geofísica 26-2100Z a 27-2100Z
The geomagnetic field was quiet to active. Solar wind speed increased to approximately 550 km/s due to the coronal hole high speed stream.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be quiet to unsettled for the next three days (28 - 30 March). Isolated active periods are possible on 28 March due to the coronal hole high speed stream.
III. Probabilidades del evento 28 Mar a 30 Mar
Clase M01%01%01%
Clase X01%01%01%
Protón01%01%01%
PCAFGreen
IV. Penticton 10.7cm flujo
  Observado       27 Mar 073
  Previsto   28 Mar-30 Mar  074/074/072
  Media de 90 Días        27 Mar 078
V. Índices Geomagnéticos A
  Observado Afr/Ap 26 Mar  007/011
  Estimado     Afr/Ap 27 Mar  012/015
  Previsto    Afr/Ap 28 Mar-30 Mar  007/010-005/005-005/005
VI. Probabilidades de Actividad Geomagnética 28 Mar a 30 Mar
A. Latitudes Medias
Activo15%15%15%
Tormenta Menor05%05%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo20%15%15%
Tormenta Menor10%05%05%
Tormenta Mayor-Severa05%01%01%

All times in UTC

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