Viendo archivo del jueves, 6 marzo 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 Mar 06 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 065 Publicado el 2200Z a las 06 Mar 2003IA. Análisis de regiones solares activas y de actividad desde 05-2100Z hasta 06-2100Z Solar activity continues at very low levels. Region 296
(N12W05) remains the largest and most complex group on the visible
disk, but has shown slow decay and very little activity over the
past 48 hours. Some developing complexity and considerable plage
fluctuations were noted in Region 301 (N22E08), but the region is
still quite small. No other significant changes were noted.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low.
Though unusually quiet for its size and complexity, Region 296 has
potential for a C-class flare and a slight chance for an M-class
event. Minor C-class flares are also possible in Region 301.
IIA. Resumen de la actividad geofísica 05-2100Z a 06-2100Z
The geomagnetic field was unsettled to active with isolated, high
latitude minor storm periods. This disturbance is due to a high
speed coronal hole stream, with solar wind speed averaging 500 to
550 km/s over the past 24 hours. The greater than 2 MeV electron
flux at geosynchronous orbit reached high levels.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to begin the period at unsettled to active levels, but
should gradually decline to mostly quiet to unsettled levels by day
two. Isolated active periods are likely on days two and three.
III. Probabilidades del evento 07 Mar a 09 Mar
| Clase M | 15% | 15% | 15% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 06 Mar 150 Previsto 07 Mar-09 Mar 145/145/145 Media de 90 Días 06 Mar 142
V. Índices Geomagnéticos A
Observado Afr/Ap 05 Mar 012/016 Estimado Afr/Ap 06 Mar 015/020 Previsto Afr/Ap 07 Mar-09 Mar 010/015-010/012-010/012
VI. Probabilidades de Actividad Geomagnética 07 Mar a 09 Mar
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 30% | 25% | 20% |
| Tormenta Menor | 10% | 05% | 05% |
| Tormenta Mayor-Severa | 05% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 40% | 30% | 30% |
| Tormenta Menor | 15% | 10% | 10% |
| Tormenta Mayor-Severa | 10% | 05% | 05% |
All times in UTC
< < Ir a la visión general diaria
Últimas noticias
miércoles, 31 diciembre 2025
Happy New Year! Celebrate with an M7.1 solar flare!
domingo, 7 diciembre 2025
M8.1 solar flare with earth-directed CME
lunes, 1 diciembre 2025
X1.9 solar flare, Coronal hole faces Earth
Últimos mensajes del foro
Más temasApoye a SpaceWeatherLive.com!
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
Hechos clima espacial
| Último evento clase X | 08/12/2025 | X1.1 |
| Último evento clase M | 31/12/2025 | M7.11 |
| Últimas tormentas geomagnéticas | 02/01/2026 | Kp5 (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| diciembre 2025 | 124 +32.2 |
| enero 2026 | 113.6 -10.4 |
| Last 30 days | 107.6 -0.4 |