Viendo archivo del sábado, 20 septiembre 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 Sep 20 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 263 Publicado el 2200Z a las 20 Sep 2003

IA. Análisis de regiones solares activas y de actividad desde 19-2100Z hasta 20-2100Z

Solar activity was low during the past 24 hours. Today's largest event was a C3.6 at 1536 UTC. There was only limited image data for this event, but it appears to have originated from newly assigned Region 464 (N05E77) which rotated into view today. Region 464 is a relatively large (360 millionths) E-type sunspot group and displayed frequent surge activity during the past 24 hours. Region 461 (N13W89), now crossing the west limb, produced the second largest event of the day, a C3 at 0512 UTC. Region 459 (S11W40) showed slow growth and occasional brightenings but was otherwise stable. LASCO images show a coronal mass ejection (CME) off the west limb, beginning at 0430 UTC. The CME does not appear to have any earthward component.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low for the next three days. Regions 464 and 459 are the most likely sources for activity. There is a slight chance for an isolated M-class flare.
IIA. Resumen de la actividad geofísica 19-2100Z a 20-2100Z
The geomagnetic field was at unsettled to minor storm levels with an isolated major storm period at some locations between 0300-0600 UTC. Geomagnetic conditions were initially unsettled from 20/2100-21/0000 UTC, but became more disturbed after 0000 UTC and remained so for the remainder of the day, with active conditions predominating. The solar wind signatures show the continued presence of a high speed coronal hole stream. In particular, the solar wind speed showed an increase around 0000 UTC up to about 700 km/s. The signature is consistent with the transition of the solar wind source from an isolated coronal hole in the western hemisphere to a southern polar extension coronal hole that crossed central meridian on 18 September. The greater than 2 MeV electron fluxes reached high levels during the past 24 hours.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be mostly active for the next 24 hours as the current coronal-hole driven disturbance continues. A slight decline to predominantly unsettled to active is expected for the second and third days. There is a fair chance for some isolated storm periods over the next three days.
III. Probabilidades del evento 21 Sep a 23 Sep
Clase M20%20%20%
Clase X01%01%01%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       20 Sep 112
  Previsto   21 Sep-23 Sep  112/115/115
  Media de 90 Días        20 Sep 120
V. Índices Geomagnéticos A
  Observado Afr/Ap 19 Sep  026/032
  Estimado     Afr/Ap 20 Sep  025/025
  Previsto    Afr/Ap 21 Sep-23 Sep  020/025-015/020-015/020
VI. Probabilidades de Actividad Geomagnética 21 Sep a 23 Sep
A. Latitudes Medias
Activo40%45%45%
Tormenta Menor25%20%20%
Tormenta Mayor-Severa10%05%05%
B. Latitudes Altas
Activo25%30%30%
Tormenta Menor35%25%25%
Tormenta Mayor-Severa20%15%10%

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