Viendo archivo del sábado, 27 febrero 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 Feb 27 2201 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 058 Publicado el 2200Z a las 27 Feb 2010

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

Solar activity was very low. No flares were detected during the forecast period.
IB. Pronóstico de la actividad solar
Solar activity is expected to be very low to low due to the return of old Region 1045 (N19, L251).
IIA. Resumen de la actividad geofísica 26-2100Z a 27-2100Z
Geomagnetic field activity was at quiet levels.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is expected to increase to quiet to unsettled levels on days one and two (28 February - 01 March) due to a recurrent coronal hole high-speed stream. Activity is expected to be at mostly quiet levels on day three (02 March) as the effects of the coronal hole wane.
III. Probabilidades del evento 28 Feb a 02 Mar
Clase M05%05%05%
Clase X01%01%01%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       27 Feb 079
  Previsto   28 Feb-02 Mar  084/084/084
  Media de 90 Días        27 Feb 081
V. Índices Geomagnéticos A
  Observado Afr/Ap 26 Feb  001/002
  Estimado     Afr/Ap 27 Feb  005/005
  Previsto    Afr/Ap 28 Feb-02 Mar  007/007-007/010-007/007
VI. Probabilidades de Actividad Geomagnética 28 Feb a 02 Mar
A. Latitudes Medias
Activo15%15%15%
Tormenta Menor01%01%01%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo20%20%20%
Tormenta Menor05%05%05%
Tormenta Mayor-Severa01%01%01%

All times in UTC

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