Viendo archivo del viernes, 14 marzo 2008

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 2008 Mar 14 2203 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 074 Publicado el 2200Z a las 14 Mar 2008

IA. Análisis de regiones solares activas y de actividad desde 13-2100Z hasta 14-2100Z

Solar activity was very low.
IB. Pronóstico de la actividad solar
Solar activity is expected to remain very low.
IIA. Resumen de la actividad geofísica 13-2100Z a 14-2100Z
The geomagnetic field ranged from quiet to active levels. The greater than 2 MeV electron flux at geosynchronous orbit remained at high levels.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be mostly quiet on day 1 (15 March) in response to a slackening of the solar wind indicated by the STEREO Behind spacecraft. Quiet to unsettled levels return on days 2 and 3 (16-17 March) as the solar wind speeds approach 600 km/s.
III. Probabilidades del evento 15 Mar a 17 Mar
Clase M01%01%01%
Clase X01%01%01%
Protón01%01%01%
PCAFGreen
IV. Penticton 10.7cm flujo
  Observado       14 Mar 070
  Previsto   15 Mar-17 Mar  070/070/070
  Media de 90 Días        14 Mar 072
V. Índices Geomagnéticos A
  Observado Afr/Ap 13 Mar  011/014
  Estimado     Afr/Ap 14 Mar  008/008
  Previsto    Afr/Ap 15 Mar-17 Mar  005/005-010/010-010/010
VI. Probabilidades de Actividad Geomagnética 15 Mar a 17 Mar
A. Latitudes Medias
Activo10%30%30%
Tormenta Menor05%05%05%
Tormenta Mayor-Severa01%05%05%
B. Latitudes Altas
Activo10%40%40%
Tormenta Menor05%10%10%
Tormenta Mayor-Severa01%05%05%

All times in UTC

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