Viendo archivo del viernes, 11 julio 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 Jul 11 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 192 Publicado el 2200Z a las 11 Jul 2003

IA. Análisis de regiones solares activas y de actividad desde 10-2100Z hasta 11-2100Z

Solar activity decreased to low levels today. Several minor B and C-class flares were observed during the period. Even though Region 397 (N12, L=028) has rotated beyond the west limb it managed to produce most of the recorded C-class activity. Region 401 (S09W05) produced the largest flare of the period, a C2.9 that occurred at 11/0739Z. This region has doubled in penumbral coverage during the interval although it remains simply structured. Region 400 (N06W65) was quiescent while undergoing steady decay. The magnetic gamma structure remains vaguely intact. Regions 405 (S10E66), 406 (S19W11), and 407 (N09E31) were newly assigned today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at low levels. With continued growth, Region 401 may become capable of producing isolated M-class flares.
IIA. Resumen de la actividad geofísica 10-2100Z a 11-2100Z
The geomagnetic field was at quiet to major storm levels. An extended period of southward Bz (-10 nT) led to the elevated conditions. An isolated period of major storm levels was observed between 11/0600 and 11/0900Z. An increase in the solar wind speed began near mid-period and is likely to be the onset of a recurrent coronal hole.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at predominantly unsettled to active levels. Isolated minor storm conditions may occur at both middle and high latitudes, especially during nighttime hours due to high speed coronal hole stream effects throughout the period. Day three may see further elevated conditions due to an anticipated transient passage from the M3.6 x-ray flare that occurred on 10 July.
III. Probabilidades del evento 12 Jul a 14 Jul
Clase M40%40%30%
Clase X01%01%01%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       11 Jul 122
  Previsto   12 Jul-14 Jul  115/110/120
  Media de 90 Días        11 Jul 125
V. Índices Geomagnéticos A
  Observado Afr/Ap 10 Jul  006/008
  Estimado     Afr/Ap 11 Jul  023/035
  Previsto    Afr/Ap 12 Jul-14 Jul  015/020-015/020-030/045
VI. Probabilidades de Actividad Geomagnética 12 Jul a 14 Jul
A. Latitudes Medias
Activo35%35%50%
Tormenta Menor20%20%30%
Tormenta Mayor-Severa10%10%15%
B. Latitudes Altas
Activo45%45%30%
Tormenta Menor30%30%40%
Tormenta Mayor-Severa15%15%25%

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