Viendo archivo del domingo, 30 marzo 2003

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 2003 Mar 30 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 089 Publicado el 2200Z a las 30 Mar 2003

IA. Análisis de regiones solares activas y de actividad desde 29-2100Z hasta 30-2100Z

Solar activity was low. Weak C-class flares were observed in Regions 321 (N05W03) and 323 (S08W15). The rapid growth and considerable C-class activity observed yesterday in Regions 318 (S13W34) and 323 has ended. Region 323, the more impressive of the two, evolved into a beta-gamma region with near 250 millionths of white light areal coverage. No significant developments were observed in the remainder of the disk or limb.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low. There is a slight chance for a low M-class flare from Regions 321 or 323.
IIA. Resumen de la actividad geofísica 29-2100Z a 30-2100Z
The geomagnetic field was unsettled to active with isolated minor storm periods at high latitudes. Solar wind signatures early this period indicate a transition from transient flow to a high speed coronal hole stream. Solar wind speed began the period near 400 km/s, but gradually increased to near 650 km/s by end of period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be unsettled to active with isolated minor storm periods. A coronal hole high speed stream will buffet the magnetosphere for most of the next three days.
III. Probabilidades del evento 31 Mar a 02 Apr
Clase M40%35%30%
Clase X05%05%05%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       30 Mar 155
  Previsto   31 Mar-02 Apr  155/150/150
  Media de 90 Días        30 Mar 133
V. Índices Geomagnéticos A
  Observado Afr/Ap 29 Mar  017/027
  Estimado     Afr/Ap 30 Mar  018/020
  Previsto    Afr/Ap 31 Mar-02 Apr  015/020-012/015-015/015
VI. Probabilidades de Actividad Geomagnética 31 Mar a 02 Apr
A. Latitudes Medias
Activo40%35%40%
Tormenta Menor20%15%20%
Tormenta Mayor-Severa05%05%05%
B. Latitudes Altas
Activo50%45%50%
Tormenta Menor30%25%30%
Tormenta Mayor-Severa10%10%10%

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