Viendo archivo del martes, 26 abril 2005
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 2005 Apr 26 2210 UTC# Prepared jointly by the U.S. Dept. of Commerce, NOAA, #Space Environment Center and the U.S. Air Force. #
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 116 Publicado el 2200Z a las 26 Apr 2005IA. Análisis de regiones solares activas y de actividad desde 25-2100Z hasta 26-2100Z Solar activity increased to low levels today. Region
756 (S06E55) appears to be a magnetically complex beta-delta sunspot
group. There were several C-class flares produced from this region
during the period, the largest was an impulsive C5 x-ray event that
occurred at 26/0441Z. A disappearing filament was observed starting
late yesterday and continued into the early part of the interval.
This event resulted in a partial halo CME which was first observed
in SOHO/LASCO C2 imagery beginning at 24/2306Z. There is a chance
this CME may become geoeffective and produce a weak glancing blow as
it passes the Earth. No new regions were numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at
low levels. There is a slight chance for an isolated M-class flare
from Region 756.
IIA. Resumen de la actividad geofísica 25-2100Z a 26-2100Z
The geomagnetic field was at quiet levels today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at predominantly quiet to unsettled levels. The
partial halo CME seen today on the southwest limb may result in
isolated periods of active conditions on 29 April.
III. Probabilidades del evento 27 Apr a 29 Apr
| Clase M | 20% | 20% | 20% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 26 Apr 091 Previsto 27 Apr-29 Apr 090/090/090 Media de 90 Días 26 Apr 090
V. Índices Geomagnéticos A
Observado Afr/Ap 25 Apr 009/011 Estimado Afr/Ap 26 Apr 003/005 Previsto Afr/Ap 27 Apr-29 Apr 005/008-005/005-012/012
VI. Probabilidades de Actividad Geomagnética 27 Apr a 29 Apr
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 15% | 25% |
| Tormenta Menor | 01% | 01% | 10% |
| Tormenta Mayor-Severa | 01% | 01% | 05% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 20% | 15% | 25% |
| Tormenta Menor | 05% | 01% | 10% |
| Tormenta Mayor-Severa | 01% | 01% | 05% |
< < Ir a la visión general diaria
Últimas noticias
lunes, 22 abril 2024
Lot's of sunspots! Big chance for major flare activity?
sábado, 23 marzo 2024
X1.1 solar flare with earth-directed CME
miércoles, 20 marzo 2024
Sunspot region 3615, G1 watch
Últimos mensajes del foro
AR3654 33Unproven theories 354Incoming Active Regions 231Growth of Cycle 25 435Unspecified geomagnetic activity 954
Más temasApoye a SpaceWeatherLive.com!
Mucha gente viene a SpaceWeatherLive para seguir la actividad del Sol o previsión de aurora, pero con esta cantidad de tráfico se incrementan los costos del servidor. ¡Considere hacer una donación si disfruta de SpaceWeatherLive para que podamos mantener el sitio web en línea!
Hechos clima espacial
| Último evento clase X | 2024/03/28 | X1.1 |
| Último evento clase M | 2024/04/29 | M3.6 |
| Últimas tormentas geomagnéticas | 2024/04/26 | Kp5+ (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| marzo 2024 | 104.9 -19.8 |
| Last 30 days | 139 +32.6 |