Viendo archivo del domingo, 4 agosto 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 Aug 04 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 216 Publicado el 2200Z a las 04 Aug 2002

IA. Análisis de regiones solares activas y de actividad desde 03-2100Z hasta 04-2100Z

Solar activity was high due to a long duration M6 x-ray event at 0955 UTC. The event was associated with activity behind the southwest limb in cotemporaneous solar image data. A faint CME could be seen in LASCO images associated with the flare with an approximate plane-of-sky speed of 500 km/s. The CME does not appear to have any earthward component. The remainder of today's solar activity consisted of occasional C-class flares. With the departure of Regions 39, 44, and 50, Region 57 is now the dominant sunspot group on the disk. Region 57 has shown growth over the past 24 hours and possesses some magnetic complexity. The group produced occasional subflare activity.
IB. Pronóstico de la actividad solar
Solar activity is expected to be mostly moderate over the next three days. There is a very slight chance, however, that one of the regions behind west limb could produce another major flare or proton producing event. Of the regions on the disk, Region 57 shows the best potential for producing an M-class event.
IIA. Resumen de la actividad geofísica 03-2100Z a 04-2100Z
The geomagnetic field ranged from quiet to minor storm levels. A period of moderately negative Bz in the solar wind occurred from about 2300-0300 UTC and led to active to minor storm conditions from 0000-0900 UTC. The source of the enhanced Bz is uncertain, but may be related to a solar sector boundary crossing from towards orientation to an away orientation which occurred during the past 24 hours.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be mostly unsettled for the next three days. There is a possibility, however, for some isolated active periods on the third and fourth days as a coronal hole will be rotating into favorable position at that time.
III. Probabilidades del evento 05 Aug a 07 Aug
Clase M50%45%45%
Clase X10%05%05%
Protón10%05%05%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       04 Aug 151
  Previsto   05 Aug-07 Aug  150/145/145
  Media de 90 Días        04 Aug 167
V. Índices Geomagnéticos A
  Observado Afr/Ap 03 Aug  011/020
  Estimado     Afr/Ap 04 Aug  015/015
  Previsto    Afr/Ap 05 Aug-07 Aug  010/010-010/010-012/015
VI. Probabilidades de Actividad Geomagnética 05 Aug a 07 Aug
A. Latitudes Medias
Activo25%25%35%
Tormenta Menor15%15%20%
Tormenta Mayor-Severa05%05%05%
B. Latitudes Altas
Activo30%30%35%
Tormenta Menor15%15%20%
Tormenta Mayor-Severa05%05%10%

All times in UTC

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