Viendo archivo del viernes, 20 diciembre 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 Dec 20 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 354 Publicado el 2200Z a las 20 Dec 2002

IA. Análisis de regiones solares activas y de actividad desde 19-2100Z hasta 20-2100Z

Solar activity increased to high levels. Along with several lesser C-class flares Region 226 (N19W16) produced an M6.8/Sf major flare (optical classification has some doubt due to the seeing conditions) at 20/1318 UTC. A Type II radio sweep (estimated shock velocity of 868 km/sec), Tenflare, and strong discrete radio busts accompanied the flare. This region has undergone little change from yesterday and retains it's beta-gamma-delta magnetic classification. Region 229 (N19W16) produced a near long duration M2.7/2n flare at 19/2153 UTC that had a Type II radio sweep with an estimated shock velocity of 668 km/sec. A Type IV radio sweep, Tenflare, and multiple discrete radio bursts were associated with the flare. SOHO/LASCO C2 and C3 imagery indicate a possible earth-bound CME as a result of this activity. Region 230 (S08E19) continues to show steady growth and was responsible for several minor C-class flares today. No new regions were numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at moderate levels. Regions 226, 229, and 230 all have the potential for M-class production. Region 226 remains capable of producing an isolated major flare.
IIA. Resumen de la actividad geofísica 19-2100Z a 20-2100Z
The geomagnetic field was at quiet to minor storm levels. The elevated conditions are due to a geoeffective recurrent positive polarity coronal hole high speed stream. The greater than 10 MeV proton flux at geosynchronous orbit became elevated following the M2.7 event early in the period while the greater than 2 MeV electron flux reached moderate levels late in the day.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at predominantly quiet to unsettled levels for day one of the forecast period. A shock passage is expected on day two due to the M2.7 event (discussed in part IA) which may result in active to minor storm conditions. By day three a return to predominantly quiet unsettled levels is expected.
III. Probabilidades del evento 21 Dec a 23 Dec
Clase M70%70%70%
Clase X15%15%15%
Protón10%10%10%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       20 Dec 197
  Previsto   21 Dec-23 Dec  195/195/185
  Media de 90 Días        20 Dec 166
V. Índices Geomagnéticos A
  Observado Afr/Ap 19 Dec  015/021
  Estimado     Afr/Ap 20 Dec  012/015
  Previsto    Afr/Ap 21 Dec-23 Dec  010/015-025/025-012/015
VI. Probabilidades de Actividad Geomagnética 21 Dec a 23 Dec
A. Latitudes Medias
Activo20%35%20%
Tormenta Menor05%25%10%
Tormenta Mayor-Severa01%10%05%
B. Latitudes Altas
Activo25%45%25%
Tormenta Menor10%30%10%
Tormenta Mayor-Severa05%10%05%

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