Viendo archivo del miércoles, 7 enero 2004

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 2004 Jan 07 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 007 Publicado el 2200Z a las 07 Jan 2004

IA. Análisis de regiones solares activas y de actividad desde 06-2100Z hasta 07-2100Z

Solar activity was high. An M4 x-ray event occurred at 0404 UTC and an M8 x-ray event occurred at 1027 UTC. Both events were from Region 537 (N07E64) and were associated with type II sweeps and CMEs off the east limb. The region rotated more fully into view today as a small (280 millionths) but bright and magnetically complex sunspot group. Region 536 (S11W02) continues to be the largest group on the disk and is maintaining its beta-gamma-delta configuration. There was some indication today that the region may be slowly decaying. Region 536 could only manage to produce a couple B-class events. Two new, small, simple regions emerged on the disk today: Region 538 (N07E04) and Region 539 (N09E29).
IB. Pronóstico de la actividad solar
Solar activity is expected to be moderate with a chance for isolated major flare activity. Region 537 is expected to remain active and Region 536 still has the potential for producing significant flare activity as well.
IIA. Resumen de la actividad geofísica 06-2100Z a 07-2100Z
The geomagnetic field ranged from unsettled to major storm levels during the past 24 hours. An enhancement in the solar wind flow was observed at ACE, beginning 2000 UTC on 06 January. The enhancement consisted of an increase in total field and in solar wind velocity, and included some extended negative Bz intervals in the -1 to -10 nT range. Although the flow was somewhat atypical (low density, high temperature), the signatures appear to be consistent with a CME led by a compression wave and expanding in low density solar wind that originated in association with the M6 x-ray event on 5 January. The slow rotation of Bz from negative to positive during the last 18 hours resulted in a decrease in geomagnetic activity during the last 5-6 hours of the period. The greater than 2 MeV electron fluxes were high during the past 24 hours.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be mostly active with some minor storm periods for 08 January based on the continued influence of a high speed solar wind stream. Mostly active conditions should predominate on 09 January and a decline to mostly unsettled levels is expected on 10 January.
III. Probabilidades del evento 08 Jan a 10 Jan
Clase M65%65%65%
Clase X15%15%15%
Protón05%05%05%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       07 Jan 119
  Previsto   08 Jan-10 Jan  120/125/125
  Media de 90 Días        07 Jan 135
V. Índices Geomagnéticos A
  Observado Afr/Ap 06 Jan  017/020
  Estimado     Afr/Ap 07 Jan  030/030
  Previsto    Afr/Ap 08 Jan-10 Jan  025/030-020/020-015/015
VI. Probabilidades de Actividad Geomagnética 08 Jan a 10 Jan
A. Latitudes Medias
Activo35%30%25%
Tormenta Menor25%20%15%
Tormenta Mayor-Severa15%10%05%
B. Latitudes Altas
Activo15%25%25%
Tormenta Menor50%35%25%
Tormenta Mayor-Severa25%20%15%

All times in UTC

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