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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 2011 Feb 14 2205 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 045 Publicado el 2200Z a las 14 Feb 2011

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

Solar activity has been moderate Region 1158 (S21W14) produce an M2/1N flare at 14/1745Z associated with a 150 sfu Tenflare and a Type II radio sweep (estimated velocity 1479 km/s). Region 1158 also produced seven C-class events the largest being a C9 at 14/1253. This region continued to grow throughout the period and is currently magnetically classified as a Beta-gamma type spotgroup with an area of 450 millionths.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low to moderate with a chance for an M5 or greater x-ray event for days one thru three (15-17 February).
IIA. Resumen de la actividad geofísica 13-2100Z a 14-2100Z
The geomagnetic field has been quiet to active. A sudden impulse was observed at 14/1600Z (12nT, as measured by the Boulder USGS magnetometer). Solar wind data from the ACE satellite indicated a shock arrival at 14/1456Z. Solar wind velocities increased to approximately 410 km/s and total field increased to around 20 nT following the shock. The source of todays activity is likely an east limb event that occurred at 11/2146Z. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be predominately quiet to unsettled with isolated active periods on day one (15 February). There is a slight chance for isolated minor storm periods on days two and three (16-17 February). The increase is forecast due to the expected return of a recurrent coronal hole high speed stream and the arrival of a CME from yesterdays M6 event.
III. Probabilidades del evento 15 Feb a 17 Feb
Clase M30%30%30%
Clase X05%05%05%
Protón01%01%01%
PCAFGreen
IV. Penticton 10.7cm flujo
  Observado       14 Feb 113
  Previsto   15 Feb-17 Feb  100/100/100
  Media de 90 Días        14 Feb 084
V. Índices Geomagnéticos A
  Observado Afr/Ap 13 Feb  001/002
  Estimado     Afr/Ap 14 Feb  007/008
  Previsto    Afr/Ap 15 Feb-17 Feb  015/018-015/018-012/012
VI. Probabilidades de Actividad Geomagnética 15 Feb a 17 Feb
A. Latitudes Medias
Activo35%35%35%
Tormenta Menor05%10%10%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo35%35%20%
Tormenta Menor10%10%05%
Tormenta Mayor-Severa05%05%01%

All times in UTC

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