Viendo archivo del martes, 15 julio 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 Jul 15 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 196 Publicado el 2200Z a las 15 Jul 2003

IA. Análisis de regiones solares activas y de actividad desde 14-2100Z hasta 15-2100Z

Solar activity was low. Today's activity consisted of a few low-level C-class flares from Region 409 (N15E41). Region 409 showed growth with the development of new spots in the trailing portion of the region. The penumbra in the region has developed to form a compact distribution of spots, suggesting that a delta configuration may form if the current trend continues. A seven degree filament near (N41E11) disappeared between 1046 UTC and 1211 UTC. New Region 411 (N16E62) was assigned today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low to moderate over the next three days, with Region 409 as the most likely source of M-class flares. There is a slight chance for major flare activity from Region 409 if the current trend continues.
IIA. Resumen de la actividad geofísica 14-2100Z a 15-2100Z
The geomagnetic field ranged from unsettled to minor storm levels. An initially active geomagnetic field reached minor storm levels from 0000-0600 UTC. Active to minor storm levels were also observed between 0900-1200 UTC. Conditions have been unsettled since 1200 UTC. The activity increase was seen in response to a jump in solar wind velocity and density accompanied by a southward turning of Bz between 14/2100 UTC and 15/0100 UTC. Solar wind conditions remained elevated for the remainder of the day, ranging mostly between 550 to 600 km/s. The solar wind data appear to be consistent with a brief interval of a co-rotating interaction region followed by a high-speed, coronal-hole-driven solar wind stream. The greater than 2 MeV electron flux reached high levels during the past 24 hours.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be active, with a chance for isolated minor storm periods, during the next 24 hours as a solar coronal hole rotates through a geoeffective position. A decline to unsettled to active levels is expected on the second day and a return to mostly unsettled levels is expected by the third day.
III. Probabilidades del evento 16 Jul a 18 Jul
Clase M40%40%40%
Clase X10%10%10%
Protón05%05%05%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       15 Jul 126
  Previsto   16 Jul-18 Jul  125/123/121
  Media de 90 Días        15 Jul 126
V. Índices Geomagnéticos A
  Observado Afr/Ap 14 Jul  013/015
  Estimado     Afr/Ap 15 Jul  020/025
  Previsto    Afr/Ap 16 Jul-18 Jul  020/025-015/020-010/015
VI. Probabilidades de Actividad Geomagnética 16 Jul a 18 Jul
A. Latitudes Medias
Activo50%40%30%
Tormenta Menor25%20%15%
Tormenta Mayor-Severa05%05%05%
B. Latitudes Altas
Activo30%30%30%
Tormenta Menor35%25%20%
Tormenta Mayor-Severa20%15%10%

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