Viendo archivo del sábado, 5 marzo 2011
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 2011 Mar 05 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 064 Publicado el 2200Z a las 05 Mar 2011IA. Análisis de regiones solares activas y de actividad desde 04-2100Z hasta 05-2100Z Solar activity was low. Region 1163 (N17W51), 1164
(N24W34) and Region 1165 (S21W52) produced several low level C-class
flares during the last 24 hours. Region 1164 and 1166 (N10E41) have
both continued to grow in white light areal coverage and spot count.
Region 1164 is a Fkc type spot group and has maintained its
Beta-Gamma-Delta magnetic configuration. Region 1166 is a Eki type
spot group and has formed a Beta-Gamma magnetic configuration.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low
with a chance for an M-class event.
IIA. Resumen de la actividad geofísica 04-2100Z a 05-2100Z
The geomagnetic field has been quiet to unsettled. Observations from
the ACE spacecraft indicate very little influence is left from the
coronal hole high speed stream which has dominated for the past five
days. Solar wind speeds are now averaging below 500 km/s. The
greater than 2 MeV electron flux at geosynchronous orbit was at high
levels throughout the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at quiet to unsettled levels with isolated periods of
active conditions, and a slight chance for minor storm periods at
high latitudes, for the next two days (06-07 March). The activity
is expected due to the possible arrival of the CME observed on 03
March. Predominately quiet conditions are expected to return on day
three (08 March).
III. Probabilidades del evento 06 Mar a 08 Mar
| Clase M | 45% | 45% | 45% |
| Clase X | 05% | 05% | 05% |
| Protón | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Penticton 10.7cm flujo
Observado 05 Mar 135 Previsto 06 Mar-08 Mar 130/130/130 Media de 90 Días 05 Mar 089
V. Índices Geomagnéticos A
Observado Afr/Ap 04 Mar 007/010 Estimado Afr/Ap 05 Mar 004/005 Previsto Afr/Ap 06 Mar-08 Mar 008/008-008/008-005/005
VI. Probabilidades de Actividad Geomagnética 06 Mar a 08 Mar
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 20% | 20% | 05% |
| Tormenta Menor | 05% | 05% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 30% | 30% | 05% |
| Tormenta Menor | 10% | 10% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
All times in UTC
< < Ir a la visión general diaria
Últimas noticias
lunes, 19 enero 2026
CME impact! S4 solar radiation storm
domingo, 18 enero 2026
X1.9 solar flare with earth-directed CME
miércoles, 31 diciembre 2025
Happy New Year! Celebrate with an M7.1 solar flare!
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 | 18/01/2026 | X1.9 |
| Último evento clase M | 19/01/2026 | M1.2 |
| Últimas tormentas geomagnéticas | 19/01/2026 | Kp9- (G4) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| diciembre 2025 | 124 +32.2 |
| enero 2026 | 103.8 -20.2 |
| Last 30 days | 109 +1.5 |