Viendo archivo del martes, 23 octubre 2012

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 2012 Oct 23 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 297 Publicado el 2200Z a las 23 Oct 2012

IA. Análisis de regiones solares activas y de actividad desde 22-2100Z hasta 23-2100Z

Solar activity has been high. Region 1598 (S12E44) produced an X1 event with an associated Tenflare and Type-II radio sweep at 23/0317Z. There was no CME observed in association with this event. Region 1598 remains the most threatening region on the disk and appears to have a Delta magnetic configuration within its trailer spots. Region 1596 (N07E06) is also moderately sized and has some magnetic complexity, but did not produce any flares during the period. Region 1593 (N15W33) produced a long-duration C3 event at 23/0821Z with an associated CME seen on STEREO-A imagery. There is not enough data available to model the CME, but at this time it does not appear likely to be geoeffective. Newly numbered Region 1599 (S09E73) appears to have a simple alpha magnetic class. The other regions on the disk either remained stable or were decaying.
IB. Pronóstico de la actividad solar
Solar activity is expected to be moderate to high with occasional M-class events, and a slight chance for an isolated X-class event for the next three days (24 - 26 Oct) with Region 1598 the most likely source.
IIA. Resumen de la actividad geofísica 22-2100Z a 23-2100Z
The geomagnetic field was quiet for the past 24 hours. Solar wind speed, as measured at the ACE spacecraft, remained steady throughout the period at approximately 370 km/s. The Bz component of the interplanetary magnetic field ranged from +/- 4 nT and the Phi angle changed to a positive sector at 22/2300Z. These signatures are consistent with a solar sector boundary crossing. The greater than 2 MeV electron flux at geosynchronous orbit was at high levels throughout the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be quiet for the next three days (24 - 26 Oct).
III. Probabilidades del evento 24 Oct a 26 Oct
Clase M75%75%75%
Clase X20%20%20%
Protón05%10%15%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       23 Oct 142
  Previsto   24 Oct-26 Oct  140/140/140
  Media de 90 Días        23 Oct 121
V. Índices Geomagnéticos A
  Observado Afr/Ap 22 Oct  002/002
  Estimado     Afr/Ap 23 Oct  007/007
  Previsto    Afr/Ap 24 Oct-26 Oct  006/005-006/005-006/005
VI. Probabilidades de Actividad Geomagnética 24 Oct a 26 Oct
A. Latitudes Medias
Activo05%05%05%
Tormenta Menor01%01%01%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%15%15%
Tormenta Menor15%15%10%
Tormenta Mayor-Severa05%05%05%

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