Viendo archivo del sábado, 28 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 28 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 362 Publicado el 2200Z a las 28 Dec 2002

IA. Análisis de regiones solares activas y de actividad desde 27-2100Z hasta 28-2100Z

Solar activity was very low. The now spotless Region 235 (N13W08) produced a subfaint flare early in the period, but has been quiet since. Occasional intensity enhancements accompanied a small increase in the size and complexity of Region 236 (N16W41). New Regions 237 (S26E00) and 238 (N09E15) were numbered today. The remaining regions are small, showing no significant changes this period. There are several large, but mostly quiescent filaments on the visible disk. Occasional motion was noted in the large filament centered near N22W12. A long duration, but low intensity X-ray enhancement was observed beginning at around 28/1700Z. This was likely associated with a strong CME that appears to have originated behind the NW limb.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low to very low. There's a chance for low C-class activity from Regions 234 (N19E19) and 236.
IIA. Resumen de la actividad geofísica 27-2100Z a 28-2100Z
The geomagnetic field was mostly unsettled to active at all latitudes. A high speed stream, associated with a large equatorial coronal hole, began late on 26 Dec and continues to buffet the magnetic field. The peak solar wind in this high speed stream exceeded 750 km/s, but has declined slowly to near 650 km/s by the end of the period. The greater than 2 MeV electron fluxes at geosynchronous orbit reached high levels.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at quiet to active levels. The high speed coronal hole stream currently impacting the geomagnetic field will gradually subside through day one. Ejecta from the CME off the NW limb late in the period today does not appear Earthbound. Expect mostly unsettled levels through days two and three of the period.
III. Probabilidades del evento 29 Dec a 31 Dec
Clase M10%10%10%
Clase X01%01%01%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       28 Dec 117
  Previsto   29 Dec-31 Dec  115/115/120
  Media de 90 Días        28 Dec 166
V. Índices Geomagnéticos A
  Observado Afr/Ap 27 Dec  022/037
  Estimado     Afr/Ap 28 Dec  020/020
  Previsto    Afr/Ap 29 Dec-31 Dec  015/015-008/010-008/010
VI. Probabilidades de Actividad Geomagnética 29 Dec a 31 Dec
A. Latitudes Medias
Activo50%30%20%
Tormenta Menor20%10%05%
Tormenta Mayor-Severa05%01%01%
B. Latitudes Altas
Activo60%40%30%
Tormenta Menor30%15%05%
Tormenta Mayor-Severa10%01%01%

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