Viendo archivo del viernes, 10 junio 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 Jun 10 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 161 Publicado el 2200Z a las 10 Jun 2005IA. Análisis de regiones solares activas y de actividad desde 09-2100Z hasta 10-2100Z Solar activity was at low levels. Region 772 (S18W84)
produced the largest flare of the period, a C2 x-ray event that
occurred at 10/0310Z. Region 775 (N08W05) underwent a slight decay
in penumbral coverage today. The southern appendage off the
dominant spot in the cluster continues to exhibit delta
characteristics. No flares were observed from this region during the
period. Region 776 (S06E07) also appeared to show a slight decay
over the interval although the region continues to depict moderate
magnetic complexity. Region 777 (N05E57) was numbered today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at
low levels. Regions 775 and 776 are both capable of producing an
isolated low level M-class flare.
IIA. Resumen de la actividad geofísica 09-2100Z a 10-2100Z
The geomagnetic field was at quiet levels. The greater than 2 MeV
electron flux at geosynchronous orbit reached high levels again
today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at predominantly quiet to unsettled levels.
Beginning late on 11 June, isolated active conditions may occur due
to the arrival of the very faint partial halo CME that occurred on 8
June.
III. Probabilidades del evento 11 Jun a 13 Jun
| Clase M | 40% | 40% | 40% |
| Clase X | 05% | 05% | 05% |
| Protón | 05% | 05% | 05% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 10 Jun 114 Previsto 11 Jun-13 Jun 110/100/100 Media de 90 Días 10 Jun 094
V. Índices Geomagnéticos A
Observado Afr/Ap 09 Jun 003/005 Estimado Afr/Ap 10 Jun 003/007 Previsto Afr/Ap 11 Jun-13 Jun 003/007-010/012-008/010
VI. Probabilidades de Actividad Geomagnética 11 Jun a 13 Jun
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 20% | 15% |
| Tormenta Menor | 05% | 10% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 20% | 30% | 20% |
| Tormenta Menor | 05% | 10% | 10% |
| Tormenta Mayor-Severa | 01% | 05% | 05% |
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
AR4366 5Broad-spectrum aurora pillars 46X1.9 CME 1339CH 17 14Do the high-resolution sunspot counts point to more complex sunspots? 36
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 | 21/01/2026 | M3.4 |
| Últimas tormentas geomagnéticas | 28/01/2026 | Kp5+ (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| diciembre 2025 | 124 +32.2 |
| enero 2026 | 119 -5 |
| Last 30 days | 119 +0.7 |