Viendo archivo del jueves, 28 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 28 2204 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 28 Jul 2005

IA. Análisis de regiones solares activas y de actividad desde 27-2100Z hasta 28-2100Z

Solar activity was moderate due to an M1 x-ray event at 0030 UTC from newly numbered Region 792 (N12E78). The event was associated with a CME off the east limb with a plane of sky speed of about 850 km/s. Region 792 is clearly the return of old Region 786, and is likely to have been the source of the recent series of CME's originating behind the east limb. The region was also responsible for the remainder of today's occasional C-class and B-class activity. Region 791 (N14W20), the only other spotted group on the Sun, was quiet and stable.
IB. Pronóstico de la actividad solar
Solar activity is expected to moderate with Region 792 as the dominant source of activity. There is also a slight chance for major flare activity from this group.
IIA. Resumen de la actividad geofísica 27-2100Z a 28-2100Z
The geomagnetic field was mostly unsettled to active with a minor storm period from 0300-0600 UTC. Solar wind data indicate the onset of a co-rotating interaction region late on the 27th followed by the onset of coronal hole stream by about midday on the 28th. Solar wind speed is currently steady at around 600 km/s. A greater than 10 MeV proton event began at 2300 UTC on the 27th and reached a maximum so far of 32 PFU at 1300 UTC on the 28th. The event continues in progress with a flux of 27 PFU at the end of the analysis interval. The main source for this event appears the shock driven by the fast CME of 27/0454 UTC. It should be noted, however, the flux levels were already enhanced prior to this event. This initial enhancement may have been caused by one or more of the earlier CME's that originated behind the east limb; for example the CME's of 26/0930 UTC, 25/1106 UTC, and 24/1418 UTC.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be mostly unsettled with a chance for some active periods for 29 July. Conditions are expected to decline to predominantly unsettled for 30 July and should be quiet to unsettled for 31 July. The greater than 10 MeV proton event is expected to end sometime on 29 July, provided that no new particles are accelerated by new activity from Region 792.
III. Probabilidades del evento 29 Jul a 31 Jul
Clase M70%70%70%
Clase X10%10%10%
Protón90%10%10%
PCAFYellow
IV. Penticton 10.7cm flujo
  Observado       28 Jul 096
  Previsto   29 Jul-31 Jul  105/110/115
  Media de 90 Días        28 Jul 096
V. Índices Geomagnéticos A
  Observado Afr/Ap 27 Jul  015/017
  Estimado     Afr/Ap 28 Jul  016/030
  Previsto    Afr/Ap 29 Jul-31 Jul  010/015-010/012-007/010
VI. Probabilidades de Actividad Geomagnética 29 Jul a 31 Jul
A. Latitudes Medias
Activo35%30%25%
Tormenta Menor20%20%15%
Tormenta Mayor-Severa05%05%05%
B. Latitudes Altas
Activo30%30%25%
Tormenta Menor25%25%15%
Tormenta Mayor-Severa10%10%05%

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