Viendo archivo del martes, 13 agosto 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 Aug 13 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 225 Publicado el 2200Z a las 13 Aug 2002

IA. Análisis de regiones solares activas y de actividad desde 12-2100Z hasta 13-2100Z

Solar activity increased to moderate levels. Region 69 (S07E50) produced an M1/1f flare at 13/1904 UTC associated with minor discrete radio emission. Region 69 showed a minor increase in penumbral coverage and remained a large, complex spot group with multiple magnetic delta configurations. Region 66 (N14E16) showed a minor increase in spots and area with some polarity mixing evident within its intermediate spots. Minor growth was also observed in Region 63 (N18W14) and Region 72 (S18W48). Region 58 (S07W89) produced a few subflares as it crossed the west limb. Two slow coronal mass ejections (estimated plane of sky velocity about 205 km/sec) occurred during the period. The source for the CMEs appeared to be beyond the southeast limb. New Region 77 (S18E48) was numbered.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at low to moderate levels. Region 69 is likely to produce isolated M-class flares during the period. There is also a slight chance for a major flare from this region.
IIA. Resumen de la actividad geofísica 12-2100Z a 13-2100Z
Geomagnetic field activity ranged from quiet to active levels until 13/0600 UTC due to coronal hole effects. Field activity decreased to quiet to unsettled levels during the rest of the period.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is expected to be at quiet to unsettled levels through the period. The greater than 2 MeV electron flux at geo-synchronous orbit may reach high levels during the first half of the forecast period.
III. Probabilidades del evento 14 Aug a 16 Aug
Clase M40%40%40%
Clase X05%05%05%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       13 Aug 192
  Previsto   14 Aug-16 Aug  190/190/195
  Media de 90 Días        13 Aug 164
V. Índices Geomagnéticos A
  Observado Afr/Ap 12 Aug  009/015
  Estimado     Afr/Ap 13 Aug  013/015
  Previsto    Afr/Ap 14 Aug-16 Aug  012/012-010/010-010/010
VI. Probabilidades de Actividad Geomagnética 14 Aug a 16 Aug
A. Latitudes Medias
Activo30%25%25%
Tormenta Menor05%05%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo35%30%30%
Tormenta Menor10%10%10%
Tormenta Mayor-Severa01%01%01%

All times in UTC

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