Viendo archivo del miércoles, 5 mayo 2010
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 2010 May 05 2201 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 125 Publicado el 2200Z a las 05 May 2010IA. Análisis de regiones solares activas y de actividad desde 04-2100Z hasta 05-2100Z Solar activity increased to moderate levels. Region
1069 (N41W40) produced an M1/Sf flare at 05/1719Z and a C8 flare at
05/1152Z, as well as occasional lesser B- and C-class flares. Region
1069 gradually increased in area and maintained a beta-gamma
magnetic configuration. Region 1066 (S26W22) produced a B4 flare at
05/1618Z associated with an EIT-wave/dimming event. New Region 1070
(N21W08), a small simple B-type spot group, was assigned late in the
period.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low
during days 1 - 3 (06 - 08 May) with a chance for isolated M-class
flares from Region 1069.
IIA. Resumen de la actividad geofísica 04-2100Z a 05-2100Z
Geomagnetic field activity was at quiet to (briefly) unsettled
levels. ACE solar wind measurements indicated Earth remained within
a subsiding coronal hole high-speed stream. Velocities gradually
decreased from 620 to 538 km/sec during the summary period. The
greater than 2 MeV electron flux at geosynchronous orbit reached
high levels during the past 24 hours.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is
expected to be at mostly quiet levels during days 1 - 2 (06 - 07
May) as the coronal hole high-speed stream continues to subside.
Field activity is expected to increase to unsettled levels on day 3
(08 May) in response to the B4 wave/dimming event mentioned above.
III. Probabilidades del evento 06 May a 08 May
| Clase M | 30% | 30% | 30% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Penticton 10.7cm flujo
Observado 05 May 083 Previsto 06 May-08 May 084/084/084 Media de 90 Días 05 May 082
V. Índices Geomagnéticos A
Observado Afr/Ap 04 May 007/010 Estimado Afr/Ap 05 May 006/008 Previsto Afr/Ap 06 May-08 May 005/005-005/005-010/010
VI. Probabilidades de Actividad Geomagnética 06 May a 08 May
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 10% | 05% | 15% |
| Tormenta Menor | 01% | 01% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 15% | 10% | 20% |
| Tormenta Menor | 05% | 01% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
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