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

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 148 Publicado el 2200Z a las 28 May 2003

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

Solar activity increased to high levels today. Region 365 (S07W32) produced two X-class flares early in the period. The first was an X1.3/2b flare that occurred at 27/2307Z with an associated Tenflare (910 sfu), Type IV, and Type II (estimated shock velocity of 607 km/s.) radio sweep. The second, larger flare, an X3.6 x-ray event which occurred at 28/0027Z that also had an associated Tenflare (1600 sfu), Type IV, and Type II (estimated 392 km/s.) radio sweep. Both flares had associated CME's (based on LASCO imagery) that appear to be Earth directed. This region continues to show good growth and remains a beta-gamma-delta magnetic complex. Little activity was noted from the rest of the disk. Region 374 (S22W59) was newly assigned today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at moderate to high levels. Region 365 is very capable of producing major flare activity.
IIA. Resumen de la actividad geofísica 27-2100Z a 28-2100Z
The geomagnetic field was at active to major storm levels. A recurrent high speed stream coronal hole is responsible for the elevated levels. The greater than 10 MeV proton fluxes have been just under event threshold levels for the past several hours of this period. The greater than 2 MeV electron fluxes at geosynchronous orbit reached moderate levels today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at predominantly active to minor storm levels through the forecast period. Transient activity from today's X-flares is expected by day two of the interval with resulting major to severe storm conditions possible. The greater than 10 MeV proton fluxes at geosynchronous orbit may reach threshold levels on day one of the period.
III. Probabilidades del evento 29 May a 31 May
Clase M75%75%75%
Clase X25%25%25%
Protón80%50%25%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       28 May 130
  Previsto   29 May-31 May  135/140/135
  Media de 90 Días        28 May 125
V. Índices Geomagnéticos A
  Observado Afr/Ap 27 May  018/026
  Estimado     Afr/Ap 28 May  025/038
  Previsto    Afr/Ap 29 May-31 May  025/025-040/050-015/025
VI. Probabilidades de Actividad Geomagnética 29 May a 31 May
A. Latitudes Medias
Activo50%35%40%
Tormenta Menor25%35%20%
Tormenta Mayor-Severa15%25%10%
B. Latitudes Altas
Activo45%30%45%
Tormenta Menor30%35%30%
Tormenta Mayor-Severa20%35%20%

All times in UTC

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