Viendo archivo del miércoles, 27 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 27 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 117 Publicado el 2200Z a las 27 Apr 2005IA. Análisis de regiones solares activas y de actividad desde 26-2100Z hasta 27-2100Z Solar activity decreased to very low levels. Region
756 (S06E42) was limited to the production of low level B-class
flares during the period. Sunspot area underwent a rapid increase
today with most the of growth being attributed to the southern delta
structure. Further magnetic analysis indicates that there may be a
delta structure just north of center in the trailing portion of the
large spot. Plage fluctuations and surging have been reported
throughout the period. Region 755 (S13W54) had several umbra
re-emerge today and remains simply structured. No new regions were
numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at
low levels. Region 756 has the capability of producing an isolated
M-class flare.
IIA. Resumen de la actividad geofísica 26-2100Z a 27-2100Z
The geomagnetic field was at quiet levels again today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at quiet to unsettled levels. There is a slight
chance that the partial halo CME observed on 25-26 April might
produce isolated active conditions on 29 April.
III. Probabilidades del evento 28 Apr a 30 Apr
| Clase M | 30% | 30% | 30% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 27 Apr 095 Previsto 28 Apr-30 Apr 100/100/100 Media de 90 Días 27 Apr 090
V. Índices Geomagnéticos A
Observado Afr/Ap 26 Apr 002/005 Estimado Afr/Ap 27 Apr 001/005 Previsto Afr/Ap 28 Apr-30 Apr 003/008-010/010-008/010
VI. Probabilidades de Actividad Geomagnética 28 Apr a 30 Apr
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 20% | 15% |
| Tormenta Menor | 01% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 15% | 20% | 20% |
| Tormenta Menor | 05% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
< < Ir a la visión general diaria
Últimas noticias
sábado, 23 marzo 2024
X1.1 solar flare with earth-directed CME
miércoles, 20 marzo 2024
Sunspot region 3615, G1 watch
jueves, 22 febrero 2024
X6.3 solar flare
Últimos mensajes del foro
C5.6 12/04/2024 CME 31AR 3637, 3638, 3643 29AR3639 10Space Weather Memes 333Where to find data for current polarity on the northern hemisphere of the sun? 27
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 | 2024/04/15 | M3.9 |
| Últimas tormentas geomagnéticas | 2024/03/25 | Kp5 (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| marzo 2024 | 104.9 -19.8 |