Viendo archivo del lunes, 14 mayo 2001
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 2001 May 14 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 134 Publicado el 2200Z a las 14 May 2001IA. Análisis de regiones solares activas y de actividad desde 13-2100Z hasta 14-2100Z Activity decreased to low levels. Region 9455 (S17W24)
remained the most active of the visible regions. It produced
isolated C-class subflares, the largest of which was a C5/Sf at
14/0324 UTC. No significant changes occurred within this region, but
mixed polarities persisted within its intermediate spots. Some
polarity mixing was also observed in the vicinity of the leading
spots of Region 9454 (N12E18), which was relatively inactive during
the period. The remaining spot groups were unremarkable, including
newly numbered Regions 9458 (S11W45), 9459 (N26W09), and 9460
(S24E60).
IB. Pronóstico de la actividad solar
Solar activity is expected to be at
low to moderate levels with a fair chance for an isolated M-class
flare from Region 9455. There will also be a slight chance for an
isolated M-class flare from Region 9454.
IIA. Resumen de la actividad geofísica 13-2100Z a 14-2100Z
Geomagnetic field activity was at unsettled to active levels until
approximately 14/0900 UTC, then decreased to quiet to unsettled
levels for the rest of the period. The greater than 2 MeV electron
flux at geosynchronous orbit increased to high levels during the
latter half of the period.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is
expected to be at quiet to unsettled levels during most of the
period with a chance for active levels at high latitudes. The
greater than 2 MeV electron flux is expected to reach high levels
during the first half of the period.
III. Probabilidades del evento 15 May a 17 May
| Clase M | 30% | 30% | 30% |
| Clase X | 05% | 05% | 05% |
| Protón | 05% | 05% | 05% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 14 May 138 Previsto 15 May-17 May 145/150/155 Media de 90 Días 14 May 167
V. Índices Geomagnéticos A
Observado Afr/Ap 13 May 017/023 Estimado Afr/Ap 14 May 013/015 Previsto Afr/Ap 15 May-17 May 012/015-012/020-007/015
VI. Probabilidades de Actividad Geomagnética 15 May a 17 May
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 25% | 20% | 15% |
| Tormenta Menor | 05% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 30% | 30% | 20% |
| Tormenta Menor | 10% | 10% | 05% |
| Tormenta Mayor-Severa | 05% | 01% | 01% |
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