Viendo archivo del martes, 9 agosto 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 Aug 09 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 221 Publicado el 2200Z a las 09 Aug 2011

IA. Análisis de regiones solares activas y de actividad desde 08-2100Z hasta 09-2100Z

Solar activity was high. Region 1263 (N17W83) produced an X6/2b flare at 09/0805Z, the largest x-ray event so far in Cycle 24. This flare was accompanied by multi-frequency radio emissions, including a Tenflare (710sfu), and Type II (1551 km/s) and IV signatures. A full halo CME was subsequently observed in LASCO C3 imagery at 09/0906Z. Initial plane-of-sky speed was estimated to be about 1000 km/s. Earlier in the period, a CME was observed in LASCO C3 imagery at 0406Z. This event was attributed to an M2/1b flare from Region 1263 at 09/03435Z. While the area of Region 1263 diminished over the last 24 hours, the longitudinal extent expanded, and the region ended the period as an Ehc type spot group with a beta-gamma-delta magnetic configuration.
IB. Pronóstico de la actividad solar
Solar activity is likely to be low to moderate. A slight chance for an isolated X-class flare, and/or proton event, remains for Day 1 (10 August). Event probabilities are expected to gradually decrease as Region 1263 rotates around the west limb.
IIA. Resumen de la actividad geofísica 08-2100Z a 09-2100Z
The geomagnetic field was quiet to unsettled through the period under the continued influence of a coronal hole high speed stream. Solar wind speed at the ACE spacecraft was approximately 600 km/s for most of the period. The Bz component of the interplanetary magnetic field was predominantly near zero. The greater than 100 MeV protons crossed the 1 pfu event threshold at 09/0825Z, reached a maximum of 2 pfu at 09/0855Z, and ended at 09/1045Z. The greater than 10 MeV protons crossed the 10 pfu event threshold at 09/0845Z, reached a maximum of 26 pfu at 09/1210Z, and ended at 09/1715Z. 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 predominantly quiet to unsettled for the next three days (10-12 August). Unsettled conditions are expected on Day 1 (10 August) as a weak remnant of the 08 August CME arrives. Currently, a return to mostly quiet conditions is expected on Days 2 and 3 (11-12 August). Analysis of the 09/0906Z CME is presently underway to determine its potential geoeffectiveness.
III. Probabilidades del evento 10 Aug a 12 Aug
Clase M60%40%20%
Clase X10%10%05%
Protón99%60%10%
PCAFYellow
IV. Penticton 10.7cm flujo
  Observado       09 Aug 098
  Previsto   10 Aug-12 Aug  095/085/085
  Media de 90 Días        09 Aug 096
V. Índices Geomagnéticos A
  Observado Afr/Ap 08 Aug  008/010
  Estimado     Afr/Ap 09 Aug  008/008
  Previsto    Afr/Ap 10 Aug-12 Aug  010/010-007/007-005/005
VI. Probabilidades de Actividad Geomagnética 10 Aug a 12 Aug
A. Latitudes Medias
Activo20%15%05%
Tormenta Menor05%05%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%20%10%
Tormenta Menor10%05%05%
Tormenta Mayor-Severa05%05%01%

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