Viendo archivo del sábado, 24 noviembre 2001

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 2001 Nov 24 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 328 Publicado el 2200Z a las 24 Nov 2001

IA. Análisis de regiones solares activas y de actividad desde 23-2100Z hasta 24-2100Z

Solar activity was low. Region 9704 (S17W63) was the principle source of flare activity and produced numerous C-class flares, the largest being a C7/Sf at 24/0553 UTC. No new regions were numbered.
IB. Pronóstico de la actividad solar
Solar activity is expected to be predominantly low to moderate. Region 9704 remains a potential source for an isolated major flare with associated proton enhancements, as it rotates through the geoeffective heliographic longitudes over the next two days.
IIA. Resumen de la actividad geofísica 23-2100Z a 24-2100Z
Geomagnetic field activity ranged from quiet to severe storm levels. The onset of storm conditions began with two sudden impulse observations: 20nt at 24/0500 UTC, followed by 80nt at 24/0555 UTC. The shock passages enhanced the already high 10 MeV proton integral flux to a peak value of 18900 pfu at 24/0555 UTC. Severe storm conditions were evident in planetary K-index values during 24/0600-1800 UTC. This event is the likely result of interaction among up to three interplanetary shock propagations from separate CME events during 21-23 November, indicated by re-analysis of shock arrival model predictions with improved event velocity data. Results suggest that the CMEs may have merged into the single interplanetary shock that passed the earth today. The 10 MeV proton event and associated polar cap absorption remained in progress at the end of the period, however the 100 MeV proton event ended at 24/1200 UTC.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity may persist with isolated active and minor storm conditions for the next 48 hours, in the wake of today's shock passage. Conditions are expected to return to quiet to unsettled conditions by day three. The 10 MeV proton event is expected to continue to wane over the next 24 hours.
III. Probabilidades del evento 25 Nov a 27 Nov
Clase M40%40%40%
Clase X10%10%10%
Protón95%50%10%
PCAFin progress
IV. Penticton 10.7cm flujo
  Observado       24 Nov 173
  Previsto   25 Nov-27 Nov  170/170/175
  Media de 90 Días        24 Nov 218
V. Índices Geomagnéticos A
  Observado Afr/Ap 23 Nov  011/012
  Estimado     Afr/Ap 24 Nov  095/105
  Previsto    Afr/Ap 25 Nov-27 Nov  030/030-018/020-012/010
VI. Probabilidades de Actividad Geomagnética 25 Nov a 27 Nov
A. Latitudes Medias
Activo35%25%20%
Tormenta Menor20%10%05%
Tormenta Mayor-Severa05%05%01%
B. Latitudes Altas
Activo35%30%20%
Tormenta Menor25%15%05%
Tormenta Mayor-Severa10%05%01%

All times in UTC

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