Viendo archivo del viernes, 3 enero 2003
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 2003 Jan 03 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 003 Publicado el 2200Z a las 03 Jan 2003IA. Análisis de regiones solares activas y de actividad desde 02-2100Z hasta 03-2100Z Solar activity was at low levels. Several low level
C-class flares occurred today. The largest optically correlated
event was a C2.0/Sf flare that occurred at 03/1445 UTC from Region
234 (N19W60) as region underwent steady decay today. Region 242
(S08E48) produced several B and C-class flares while showing areal
growth of spot complex through the period. An eruptive prominence
on the west limb (N22W90) occurred at 03/1506 UTC producing a CME
seen on NASA/LASCO imagery that does not appear to be earth
directed. Regions 243 (S19W34), 244 (S15E58), and 245 (N12E74) were
newly assigned today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at
low levels. A very slight chance of an isolated low level M-class
flare is possible from Region 242.
IIA. Resumen de la actividad geofísica 02-2100Z a 03-2100Z
The geomagnetic field was predominantly quiet to unsettled. Isolated
active to minor storm conditions were observed between 03/1500 to
1800 UTC due to the effects of a favorably positioned coronal hole.
The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels during the past 24 hours.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at predominantly unsettled to active levels on day
one of the forecast period due to high speed stream coronal hole.
Days two and three should see a return to quiet to unsettled
conditions as the geo-effective coronal hole wanes.
III. Probabilidades del evento 04 Jan a 06 Jan
| Clase M | 20% | 20% | 20% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 03 Jan 138 Previsto 04 Jan-06 Jan 135/140/145 Media de 90 Días 03 Jan 164
V. Índices Geomagnéticos A
Observado Afr/Ap 02 Jan 005/008 Estimado Afr/Ap 03 Jan 010/015 Previsto Afr/Ap 04 Jan-06 Jan 012/015-010/015-005/010
VI. Probabilidades de Actividad Geomagnética 04 Jan a 06 Jan
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 25% | 25% | 15% |
| Tormenta Menor | 10% | 05% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 30% | 30% | 25% |
| Tormenta Menor | 10% | 10% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
All times in UTC
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