Viendo archivo del martes, 11 mayo 2010

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 2010 May 11 2201 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 131 Publicado el 2200Z a las 11 May 2010

IA. Análisis de regiones solares activas y de actividad desde 10-2100Z hasta 11-2100Z

Solar activity was very low. The visible disk remained spotless.
IB. Pronóstico de la actividad solar
Solar activity is expected to remain at very low levels.
IIA. Resumen de la actividad geofísica 10-2100Z a 11-2100Z
The geomagnetic field was at quiet to unsettled levels. A solar sector boundary crossing from negative (toward) to positive (away) was evident in ACE SWEPAM signatures at about 11/0130Z. Shortly afterwards, solar wind velocity gradually increased from about 350 km/s to near 400 km/s by 0600Z, while the Bz component of the interplanetary magnetic field turned southward (-5 nT). These signatures were consistent with a co-rotating interaction region in advance of a coronal hole high speed wind stream. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels.
IIB. Pronóstico de la actividad geofísica
The geomagetic field is expected to be at quiet to unsettled levels, with isolated active periods, all three days of the forecast period (12 - 14 May). This activity is due to a series of coronal hole high speed wind streams that are located in both solar hemispheres.
III. Probabilidades del evento 12 May a 14 May
Clase M01%01%01%
Clase X01%01%01%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       11 May 074
  Previsto   12 May-14 May  074/073/073
  Media de 90 Días        11 May 081
V. Índices Geomagnéticos A
  Observado Afr/Ap 10 May  004/005
  Estimado     Afr/Ap 11 May  008/008
  Previsto    Afr/Ap 12 May-14 May  010/010-008/008-008/008
VI. Probabilidades de Actividad Geomagnética 12 May a 14 May
A. Latitudes Medias
Activo30%25%25%
Tormenta Menor10%05%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo35%30%30%
Tormenta Menor15%10%10%
Tormenta Mayor-Severa01%01%01%

All times in UTC

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