Viendo archivo del miércoles, 11 mayo 2011

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 May 11 2200 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 2011

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

Solar activity was very low. A B8 x-ray flare occurred at 11/0243Z, likely associated with a filament eruption between Regions 1205 (N14W75) and 1207 (N21W51). The flare was associated with a Type II radio sweep and a partial-halo coronal mass ejection (CME). The CME had an estimated plane-of-sky speed of 420 km/s, based on SOHO/LASCO images. No significant changes occurred in any of the spotted regions. New Region 1212 (S13E46) was numbered and was classified as a single-spot Axx region.
IB. Pronóstico de la actividad solar
Solar activity is expected to be very low during the period (12 - 14 May) with a chance for isolated C-class flares.
IIA. Resumen de la actividad geofísica 10-2100Z a 11-2100Z
Geomagnetic activity was at quiet to unsettled levels. ACE solar wind data indicated Earth remained under the influence of a recurrent coronal hole high-speed stream (CH HSS). Solar wind speeds ranged from 352 to 414 km/sec with no discernible trend. A slight increase in the greater than 10 MeV proton flux occurred in the wake of the B8 flare mentioned above.
IIB. Pronóstico de la actividad geofísica
Geomagnetic activity is expected to be at unsettled to active levels on day 1 (12 May) with a chance for minor storm levels as the CH HSS persists. The CME observed late on 09 May may also disturb the field on May 12. Activity is expected to decrease to quiet to unsettled levels on day 2 (13 May) as the CH HSS begins to subside. Activity is expected to decrease to quiet levels on day 3 (14 May). The CME observed today is not expected to affect the field during the forecast period.
III. Probabilidades del evento 12 May a 14 May
Clase M10%10%10%
Clase X01%01%01%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       11 May 094
  Previsto   12 May-14 May  095/095/095
  Media de 90 Días        11 May 110
V. Índices Geomagnéticos A
  Observado Afr/Ap 10 May  005/008
  Estimado     Afr/Ap 11 May  005/005
  Previsto    Afr/Ap 12 May-14 May  015/015-008/010-005/005
VI. Probabilidades de Actividad Geomagnética 12 May a 14 May
A. Latitudes Medias
Activo35%10%05%
Tormenta Menor15%05%01%
Tormenta Mayor-Severa05%01%01%
B. Latitudes Altas
Activo40%15%10%
Tormenta Menor20%10%01%
Tormenta Mayor-Severa10%01%01%

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