Viendo archivo del lunes, 2 diciembre 2002
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 2002 Dec 02 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 336 Publicado el 2200Z a las 02 Dec 2002IA. Análisis de regiones solares activas y de actividad desde 01-2100Z hasta 02-2100Z Solar activity was low. Region 208 (N10E35) produced
the largest event of the period, a C9/Sf flare at 02/1927 UTC. This
region has undergone minor growth in size and spot count and shown
an increase in magnetic complexity over the past 24 hours. Region
207 (S20E06) remains the largest region on the visible disk, and
produced a C1/Sf flare at 02/2033 UTC. An impressive partial-halo
CME was visible over the northwest limb in SOHO/LASCO C2 imagery
starting at about 02/1750 UTC, but a lack in corresponding
observations of notable x-ray enhancement or optical flare activity
suggests a likely backside source for this event. Two new regions
were numbered today: Region 211 (S08E04) and Region 212 (N13E75).
IB. Pronóstico de la actividad solar
Solar activity is expected to be
predominantly low, with a slight chance for moderate flare activity
during the next three days. Region 208 appears to be the most
likely source for possible M-class activity during the period.
IIA. Resumen de la actividad geofísica 01-2100Z a 02-2100Z
The geomagnetic field was quiet to unsettled. The greater than 2 MeV
electron flux at geosynchronous orbit again reached high levels
today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at quiet to unsettled levels for the next three days.
Greater than 2 MeV electron flux at geosynchronous orbit is likely
to persist at high levels for the next one to three days.
III. Probabilidades del evento 03 Dec a 05 Dec
| Clase M | 30% | 30% | 30% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 02 Dec 146 Previsto 03 Dec-05 Dec 155/160/175 Media de 90 Días 02 Dec 169
V. Índices Geomagnéticos A
Observado Afr/Ap 01 Dec 016/016 Estimado Afr/Ap 02 Dec 010/015 Previsto Afr/Ap 03 Dec-05 Dec 012/015-010/012-005/008
VI. Probabilidades de Actividad Geomagnética 03 Dec a 05 Dec
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 25% | 20% | 15% |
| Tormenta Menor | 10% | 05% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 30% | 25% | 20% |
| Tormenta Menor | 15% | 10% | 05% |
| Tormenta Mayor-Severa | 05% | 01% | 01% |
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