Viendo archivo del viernes, 9 mayo 2008
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 2008 May 09 2203 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 130 Publicado el 2200Z a las 09 May 2008IA. Análisis de regiones solares activas y de actividad desde 08-2100Z hasta 09-2100Z Solar activity was very low. No flares were detected.
The visible disk remained spotless.
IB. Pronóstico de la actividad solar
Solar activity is expected to be very
low.
IIA. Resumen de la actividad geofísica 08-2100Z a 09-2100Z
The geomagnetic field was quiet. The greater than 2 MeV electron flux
at geosynchronous orbit was high during most of the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be quiet throughout the period (10 - 12 May).
III. Probabilidades del evento 10 May a 12 May
| Clase M | 01% | 01% | 01% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Penticton 10.7cm flujo
Observado 09 May 067 Previsto 10 May-12 May 068/070/070 Media de 90 Días 09 May 071
V. Índices Geomagnéticos A
Observado Afr/Ap 08 May 003/004 Estimado Afr/Ap 09 May 003/005 Previsto Afr/Ap 10 May-12 May 005/005-005/005-005/005
VI. Probabilidades de Actividad Geomagnética 10 May a 12 May
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 10% | 10% | 10% |
| Tormenta Menor | 05% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 15% | 15% | 15% |
| Tormenta Menor | 05% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
All times in UTC
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