Viendo archivo del lunes, 11 junio 2001
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 2001 Jun 11 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 162 Publicado el 2200Z a las 11 Jun 2001IA. Análisis de regiones solares activas y de actividad desde 10-2100Z hasta 11-2100Z Solar activity was low. The largest events of the
period were the successive C5 and C7 x-ray bursts at 11/0451Z and
11/0552Z respectively. These events appeared to be associated with
activity on the SE limb near new Region 9501 (S14E69), and a
filament eruption south of Region 9488 (S19W45). CME's were observed
with both events, but did not appear earthbound. Region 9494
(S08W69) was responsible for some minor C-class activity, but though
maintaining moderate complexity and size, flare output has decreased
considerably. Three new regions were numbered today - Regions 9499
(N18E17), 9500 (N10E71), and 9501, making a total of 15 spot groups
on the visible disk..
IB. Pronóstico de la actividad solar
Solar activity is expected to be low
to moderate. A small chance for an M-class flare exist in several
regions, primarily in Region 9494.
IIA. Resumen de la actividad geofísica 10-2100Z a 11-2100Z
The geomagnetic field was quiet to unsettled. The greater than 2 MeV
electrons were at moderate levels for the latter half of the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to continue at quiet to unsettled levels.
III. Probabilidades del evento 12 Jun a 14 Jun
| Clase M | 40% | 40% | 30% |
| Clase X | 05% | 05% | 01% |
| Protón | 05% | 05% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 11 Jun 162 Previsto 12 Jun-14 Jun 160/155/155 Media de 90 Días 11 Jun 169
V. Índices Geomagnéticos A
Observado Afr/Ap 10 Jun 013/020 Estimado Afr/Ap 11 Jun 007/012 Previsto Afr/Ap 12 Jun-14 Jun 008/010-008/010-008/010
VI. Probabilidades de Actividad Geomagnética 12 Jun a 14 Jun
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 20% | 20% | 20% |
| Tormenta Menor | 05% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 25% | 25% | 25% |
| Tormenta Menor | 05% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
All times in UTC
< < Ir a la visión general diaria
Últimas noticias
domingo, 1 febrero 2026
Complex sunspot region 4366
lunes, 19 enero 2026
CME impact! S4 solar radiation storm
domingo, 18 enero 2026
X1.9 solar flare with earth-directed CME
Últimos mensajes del foro
Yes, we really went to the moon before. 5AR4366 1029Feb 8-9 CMEs 28Current Farside Activity 374Do the high-resolution sunspot counts point to more complex sunspots? 63
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 | 04/02/2026 | X4.3 |
| Último evento clase M | 12/02/2026 | M1.4 |
| Últimas tormentas geomagnéticas | 05/02/2026 | Kp5+ (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| enero 2026 | 112.6 -11.4 |
| febrero 2026 | 125.3 +12.7 |
| Last 30 days | 130.4 +32.7 |