Viendo archivo del sábado, 12 enero 2002

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 2002 Jan 12 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 012 Publicado el 2200Z a las 12 Jan 2002

IA. Análisis de regiones solares activas y de actividad desde 11-2100Z hasta 12-2100Z

Solar activity has been moderate due to four M-class events during the past 24 hours. Region 9775 (S05E30) produced three of these: an M1/Sf at 0322 UTC, an M1/1n at 1519 UTC, and an M1/Sf at 1929 UTC. The region has not changed size significantly, but appears to be active due to the emergence of new magnetic flux. The group currently has a relatively complex magnetic configuration (beta-gamma). The fourth M-class event was an M3 at 1843 UTC: this event was associated with erupting prominence activity on the west limb near S17. Region 9773 (N15W46) continues to be the largest sunspot group on the disk. This group did not show much change and managed to produce a few subflares during the past 24 hours.
IB. Pronóstico de la actividad solar
Solar activity is expected to be moderate. Regions 9773, 9775, and 9778 are the most likely sources for M-class flares. There continues to be a slight chance for a major flare or proton producing flare from Region 9773.
IIA. Resumen de la actividad geofísica 11-2100Z a 12-2100Z
The geomagnetic field was unsettled to active during the past 24 hours. The enhanced level of activity was due to continued effects from a coronal hole associated high speed solar wind stream. The solar wind velocity showed an overall decreasing trend today, suggesting that the coronal hole effects should not last much longer. The greater than 10 MeV proton event that began on 10/2045 UTC continues in progress: flux levels decayed throughout the day and had reached 16.1 PFU at forecast issue time.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to decrease to mostly unsettled levels for the next two days as the current enhanced solar wind should subside soon. Quiet to unsettled levels are expected by day three. LASCO observations do not show any CMEs to be associated with today's solar flare activity.
III. Probabilidades del evento 13 Jan a 15 Jan
Clase M70%70%70%
Clase X20%20%20%
Protón50%20%20%
PCAFin progress
IV. Penticton 10.7cm flujo
  Observado       12 Jan 233
  Previsto   13 Jan-15 Jan  235/240/240
  Media de 90 Días        12 Jan 224
V. Índices Geomagnéticos A
  Observado Afr/Ap 11 Jan  012/021
  Estimado     Afr/Ap 12 Jan  015/015
  Previsto    Afr/Ap 13 Jan-15 Jan  012/012-012/010-005/008
VI. Probabilidades de Actividad Geomagnética 13 Jan a 15 Jan
A. Latitudes Medias
Activo25%25%20%
Tormenta Menor10%10%05%
Tormenta Mayor-Severa05%05%01%
B. Latitudes Altas
Activo25%25%20%
Tormenta Menor15%15%10%
Tormenta Mayor-Severa05%05%01%

All times in UTC

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