Viendo archivo del sábado, 8 abril 2000
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 2000 Apr 08 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 099 Publicado el 2200Z a las 08 APR 2000IA. Análisis de regiones solares activas y de actividad desde 07-2100Z hasta 08-2100Z SOLAR ACTIVITY HAS BEEN MODERATE. REGION 8948 (S15E14)
PRODUCED AN M2/1B FLARE AT 0240Z AND AN M1/1N AT 2046Z. THIS REGION
HAS CONTINUED TO GROW AND HAS A COMPLICATED MAGNETIC STRUCTURE
INCLUDING A SMALL DELTA SPOT. NEARLY ALL OF TODAY'S OBSERVED FLARE
ACTIVITY CAME FROM THIS GROUP. REGION 8951 (N13E64) ROTATED MORE
FULLY INTO VIEW AS A D-TYPE SUNSPOT GROUP. REGION 8949 (S19E43)
EXHIBITED GROWTH BUT WAS STABLE. A CME WAS OBSERVED TO ENTER THE
LASCO C2 FIELD OF VIEW AT 1554Z TODAY: THE MATERIAL WAS CONSTRAINED
TO A RELATIVELY SMALL ANGLE OFF THE SOUTHWEST LIMB, AND DISK
OBSERVATIONS INDICATED THAT THE SOURCE REGION WAS JUST BEHIND WEST
LIMB.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE
MODERATE. REGION 8948 SHOWS FAIR-GOOD POTENTIAL FOR PRODUCING
ADDITIONAL M-CLASS FLARES.
IIA. Resumen de la actividad geofísica 07-2100Z a 08-2100Z
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED AT MID-LATITUDES AND WAS
QUIET TO ACTIVE AT HIGH LATITUDES. THE HIGH LATITUDE ACTIVE PERIODS
OCCURRED FROM 0600-1200Z. SOLAR WIND SPEED REMAINS ELEVATED (500-550
KM/S), BUT THE DENSITY IS LOW AND THE MAGNETIC FIELD INTENSITY IS
WEAK.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE MOSTLY UNSETTLED FOR THE NEXT THREE DAYS.
III. Probabilidades del evento 09 APR a 11 APR
| Clase M | 60% | 60% | 60% |
| Clase X | 05% | 05% | 05% |
| Protón | 05% | 05% | 05% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 08 APR 182 Previsto 09 APR-11 APR 180/180/175 Media de 90 Días 08 APR 186
V. Índices Geomagnéticos A
OBSERVED AFR/AP 07 APR 034/050 ESTIMATED AFR/AP 08 APR 015/015 PREDICTED AFR/AP 09 APR-11 APR 012/010-010/010-008/008
VI. Probabilidades de Actividad Geomagnética 09 APR a 11 APR
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 20% | 15% | 10% |
| Tormenta Menor | 10% | 05% | 05% |
| Tormenta Mayor-Severa | 05% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 30% | 20% | 15% |
| Tormenta Menor | 15% | 10% | 05% |
| Tormenta Mayor-Severa | 10% | 05% | 05% |
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
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 | 05/02/2026 | M1.1 |
| 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 | 140.8 +28.2 |
| Last 30 days | 124.6 +17.7 |