Viendo archivo del martes, 27 julio 2004

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 2004 Jul 27 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 209 Publicado el 2200Z a las 27 Jul 2004

IA. Análisis de regiones solares activas y de actividad desde 26-2100Z hasta 27-2100Z

Solar activity was moderate. Region 652 (N07W62) produced three M1 flares this period. Region 652 continues to slowly decay as it approaches the west limb. It still maintains considerable size and a complex delta configuration. No other significant changes were observed on the disk or limb.
IB. Pronóstico de la actividad solar
Solar activity is expected to be moderate. Continued M-class activity is expected from Region 652 and there is a slight chance for a major flare.
IIA. Resumen de la actividad geofísica 26-2100Z a 27-2100Z
The geomagnetic field ranged from unsettled to severe storming. A strong sudden impulse (SI) of 95 Nt was observed on the Boulder magnetometer at 26/2228Z. This SI followed the very fast (~31 hours) transit of the full halo CME associated with the long duration M1 flare on 25/1514Z. Solar wind speed increased from the already elevated levels near 600 km/s to over 1050 km/s. After approximately four hours of fluctuating between -15 and +15 nT, the IMF Bz rotated strong southward and ranged from -15 to -25 nT for about 15 hours. The fast solar wind speed and southward Bz combined to produce severe geomagnetic storm levels at all latitudes from 27/0000Z to 27/1500Z. Solar wind speed was still near 800 km/s by the end of the period and the disturbance had declined to minor storm levels. The greater than 10 MeV proton event that began on 25/1855Z is still in progress. A rapid, short-lived increase in the greater than 10 MeV protons to 2,090 pfu occurred with the shock passage. Protons quickly declined and were straddling the 10 pfu alert threshold by the end of the period. The greater than 2 MeV electrons at geosynchronous orbit were at high levels.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to range from quiet to major storm levels. The most disturbed periods are expected during the first half of day one as the current major disturbance subsides. Mostly quiet to unsettled conditions are expected on 29 - 30 July.
III. Probabilidades del evento 28 Jul a 30 Jul
Clase M55%40%10%
Clase X10%05%05%
Protón99%10%05%
PCAFyellow
IV. Penticton 10.7cm flujo
  Observado       27 Jul 118
  Previsto   28 Jul-30 Jul  110/105/090
  Media de 90 Días        27 Jul 106
V. Índices Geomagnéticos A
  Observado Afr/Ap 26 Jul  026/031
  Estimado     Afr/Ap 27 Jul  120/180
  Previsto    Afr/Ap 28 Jul-30 Jul  020/025-010/015-008/010
VI. Probabilidades de Actividad Geomagnética 28 Jul a 30 Jul
A. Latitudes Medias
Activo50%35%20%
Tormenta Menor25%05%05%
Tormenta Mayor-Severa15%01%01%
B. Latitudes Altas
Activo50%40%20%
Tormenta Menor30%10%05%
Tormenta Mayor-Severa20%05%01%

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