Viendo archivo del domingo, 2 febrero 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 Feb 02 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 033 Publicado el 2200Z a las 02 Feb 2003

IA. Análisis de regiones solares activas y de actividad desde 01-2100Z hasta 02-2100Z

Solar activity was low. Region 276 (S14E66) produced numerous C-flares during the past 24 hours. The largest of these was a C2/Sf at 0334 UTC. The region appears to be an E-type sunspot group with an area of about 240 millionths. Region 274 (S06E05) showed some growth during the past 24 hours, and displayed occasional brightenings but did not produce any flare level activity. The remaining solar active regions were quiet and stable.
IB. Pronóstico de la actividad solar
Solar activity is expected to be mostly low, but there is a fair chance for an isolated M-class event from Region 276 sometime during the next three days.
IIA. Resumen de la actividad geofísica 01-2100Z a 02-2100Z
The geomagnetic field ranged from active to minor storm levels with a period of major storm levels at high latitudes from 1200-1500 UTC. The enhanced solar wind flow which was reported yesterday continued during the past 24 hours, with speeds in the 500 to 700 km/s range and total magnetic field around 10 to 12 nT. Occasional periods of southward turning of the interplanetary magnetic field were associated with times of enhanced geomagnetic activity.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be mostly unsettled to active during the next 24 hours, but there will probably be some periods of minor storm levels as the current disturbance persists partway into the first day. A decrease to mostly unsettled is expected for the second day. An increase to unsettled to active is anticipated on the third day in response to a favorably positioned coronal hole.
III. Probabilidades del evento 03 Feb a 05 Feb
Clase M35%35%35%
Clase X05%05%05%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       02 Feb 127
  Previsto   03 Feb-05 Feb  130/135/140
  Media de 90 Días        02 Feb 155
V. Índices Geomagnéticos A
  Observado Afr/Ap 01 Feb  010/013
  Estimado     Afr/Ap 02 Feb  028/050
  Previsto    Afr/Ap 03 Feb-05 Feb  015/030-010/015-012/020
VI. Probabilidades de Actividad Geomagnética 03 Feb a 05 Feb
A. Latitudes Medias
Activo35%25%30%
Tormenta Menor20%15%20%
Tormenta Mayor-Severa10%05%05%
B. Latitudes Altas
Activo40%30%35%
Tormenta Menor25%15%20%
Tormenta Mayor-Severa15%05%10%

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