Viendo archivo del viernes, 21 marzo 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 Mar 21 2203 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 081 Publicado el 2200Z a las 21 Mar 2008IA. Análisis de regiones solares activas y de actividad desde 20-2100Z hasta 21-2100Z Solar activity was at very low levels. The visible
solar disk remained spotless.
IB. Pronóstico de la actividad solar
Solar activity is expected to continue
at very low levels.
IIA. Resumen de la actividad geofísica 20-2100Z a 21-2100Z
The geomagnetic field was at quiet levels.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to remain at predominately quiet levels.
III. Probabilidades del evento 22 Mar a 24 Mar
| Clase M | 01% | 01% | 01% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Penticton 10.7cm flujo
Observado 21 Mar 068 Previsto 22 Mar-24 Mar 070/070/070 Media de 90 Días 21 Mar 072
V. Índices Geomagnéticos A
Observado Afr/Ap 20 Mar 007/008 Estimado Afr/Ap 21 Mar 005/005 Previsto Afr/Ap 22 Mar-24 Mar 005/005-005/005-005/005
VI. Probabilidades de Actividad Geomagnética 22 Mar a 24 Mar
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 05% | 05% | 05% |
| Tormenta Menor | 01% | 01% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 05% | 05% | 05% |
| Tormenta Menor | 01% | 01% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
All times in UTC
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