Viendo archivo del lunes, 14 octubre 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 Oct 14 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 287 Publicado el 2200Z a las 14 Oct 2002

IA. Análisis de regiones solares activas y de actividad desde 13-2100Z hasta 14-2100Z

Solar activity increased to moderate. A long-duration M2/Sf event occurred early in the period peaking at 14/0010 UTC, from bright plage just east of the large spot in Region 159 (S11E57). This event was accompanied by a large CME evident in SOHO/LASCO imagery, with an estimated plane-of-sky velocity of about 850 km/s. Region 159 also produced a C4/Sf event at 14/0945 UTC. A Type-II radio sweep of estimated velocity 743 km/s was observed at 14/1429 UTC, in association with a small impulsive C1 flare, and followed shortly thereafter by a very long-lived enhancement in x-ray flux that began at about 14/1520 UTC, and remained in progress at the end of the period. Available H-alpha imagery revealed no apparent source for this activity, and SOHO EIT and LASCO data were mostly unavailable for the period. The lack of subsequent particle enhancement from this potential CME event seems to suggest an east-limb source for this activity. New Region 160 (S20E54) was numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low to moderate for the next three days.
IIA. Resumen de la actividad geofísica 13-2100Z a 14-2100Z
The geomagnetic field ranged from quiet to major storm levels. An extended interval of active conditions, with an isolated period of major storming at high latitudes, appeared to occur primarily due to a sustained strong southward orientation of Bz, and a slow increase in solar wind speed. Other solar wind data suggest an overall pattern of a CIR evolving toward to a weak high speed stream pattern near the end of the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be quiet to active for the early part of the forecast period, with mostly quiet to unsettled conditions by the end of day one and into day two. By day three, some CME passage effects may occur in response to the solar activity described above, and may cause isolated active or minor storm conditions by the end of the period.
III. Probabilidades del evento 15 Oct a 17 Oct
Clase M30%30%30%
Clase X05%05%05%
Protón05%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       14 Oct 181
  Previsto   15 Oct-17 Oct  175/175/165
  Media de 90 Días        14 Oct 182
V. Índices Geomagnéticos A
  Observado Afr/Ap 13 Oct  006/010
  Estimado     Afr/Ap 14 Oct  017/026
  Previsto    Afr/Ap 15 Oct-17 Oct  015/018-012/012-015/025
VI. Probabilidades de Actividad Geomagnética 15 Oct a 17 Oct
A. Latitudes Medias
Activo25%20%30%
Tormenta Menor05%05%10%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo30%25%35%
Tormenta Menor10%05%15%
Tormenta Mayor-Severa01%01%05%

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