Viendo archivo del sábado, 16 julio 2005

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 2005 Jul 16 2200 UTC
# Prepared jointly by the U.S. Dept. of Commerce, NOAA, #Space Environment Center and the U.S. Air Force. #

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 197 Publicado el 2200Z a las 16 Jul 2005

IA. Análisis de regiones solares activas y de actividad desde 15-2100Z hasta 16-2100Z

Solar activity was at moderate levels. Region 790 (S10W80) produced an impulsive M1 x-ray flare at 16/0338Z. It was also the source for a very long duration C7 flare that occurred between 15/2010Z and 16/0005Z. A Type II radio sweep occurred in association with a C2 flare that occurred at 16/0714Z from Region 790, although LASCO imagery showed little associated CME activity. No new regions were numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at low levels. Region 790 remains capable of producing an isolated M-class flare.
IIA. Resumen de la actividad geofísica 15-2100Z a 16-2100Z
The geomagnetic field was at predominantly quiet to unsettled levels. An active period occurred at the Boulder magnetometer between 16/0600 and 0900Z. A weak transient signature was observed at the ACE spacecraft near 16/0100Z with no significant geomagnetic effects resulting. The greater than 10 MeV proton event that began on 14/0245Z, had a peak flux of 134 pfu at 15/0345Z, remains in-progress. The proton flux has been on a gradual decrease and was near 11 pfu at the end of the period. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels again today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at quiet to active levels. Isolated minor storm conditions may be possible with the onset of the anticipated transient from the CME activity that occurred on 14 July. The greater than 10 MeV proton event is expected to end early in the period on 17 July.
III. Probabilidades del evento 17 Jul a 19 Jul
Clase M15%05%01%
Clase X05%01%01%
Protón99%15%01%
PCAFyellow
IV. Penticton 10.7cm flujo
  Observado       16 Jul 076
  Previsto   17 Jul-19 Jul  075/075/075
  Media de 90 Días        16 Jul 097
V. Índices Geomagnéticos A
  Observado Afr/Ap 15 Jul  004/006
  Estimado     Afr/Ap 16 Jul  008/008
  Previsto    Afr/Ap 17 Jul-19 Jul  010/012-005/010-008/008
VI. Probabilidades de Actividad Geomagnética 17 Jul a 19 Jul
A. Latitudes Medias
Activo20%15%20%
Tormenta Menor10%05%05%
Tormenta Mayor-Severa05%01%01%
B. Latitudes Altas
Activo30%20%20%
Tormenta Menor15%10%05%
Tormenta Mayor-Severa05%05%01%

All times in UTC

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