Viendo archivo del lunes, 26 junio 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 Jun 26 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 178 Publicado el 2200Z a las 26 JUN 2000IA. Análisis de regiones solares activas y de actividad desde 25-2100Z hasta 26-2100Z SOLAR ACTIVITY DECREASED TO LOW LEVELS. OCCASIONAL,
MOSTLY LOW-LEVEL C-CLASS SUBFLARES OCCURRED, MOST OF WHICH WERE
PRODUCED BY REGION 9054 (N12W18). THIS REGION IS A MEDIUM-SIZED,
MIXED-POLARITY (BETA-GAMMA) GROUP THAT HAS GRADUALLY DEVELOPED
DURING THE LAST FEW DAYS. IT WAS THE LIKELY SOURCE (BASED ON
SOHO/EIT IMAGES) FOR A C4 X-RAY FLARE AT 26/0157Z ASSOCIATED WITH A
WEAK TYPE II RADIO SWEEP (EST. SHOCK VELOCITY 800 KM/SEC) AND A
POSSIBLE PARTIAL-HALO CME. REGIONS 9046 (N20W75) AND 9049 (N16W09)
DECAYED SLIGHTLY, WHILE THE REMAINING REGIONS WERE STABLE. NEW
REGION 9063 (N24E41) WAS NUMBERED.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE AT
LOW TO MODERATE LEVELS. OCCASIONAL C-CLASS SUBFLARES ARE EXPECTED.
REGION 9054 APPEARS CAPABLE OF PRODUCING AN ISOLATED M-CLASS FLARE.
IIA. Resumen de la actividad geofísica 25-2100Z a 26-2100Z
GEOMAGNETIC FIELD ACTIVITY INCREASED TO UNSETTLED TO ACTIVE LEVELS
WITH BRIEF MINOR TO MAJOR STORM PERIODS AT HIGH LATITUDES.
IIB. Pronóstico de la actividad geofísica
GEOMAGNETIC FIELD ACTIVITY IS
EXPECTED TO REMAIN AT UNSETTLED TO ACTIVE LEVELS DURING 27 - 28 JUNE
WITH BRIEF STORM LEVELS POSSIBLE AT HIGH LATITUDES. FIELD ACTIVITY
IS EXPECTED TO DECLINE TO QUIET TO UNSETTLED LEVELS DURING THE LAST
DAY OF THE PERIOD. THE GREATER THAN 2 MEV ELECTRON FLUX AT
GEOSYNCHRONOUS ORBIT IS EXPECTED TO INCREASE TO MODERATE TO HIGH
LEVELS DURING THE PERIOD.
III. Probabilidades del evento 27 JUN a 29 JUN
| Clase M | 30% | 30% | 30% |
| Clase X | 05% | 05% | 05% |
| Protón | 01% | 01% | 01% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 26 JUN 177 Previsto 27 JUN-29 JUN 170/165/165 Media de 90 Días 26 JUN 185
V. Índices Geomagnéticos A
OBSERVED AFR/AP 25 JUN 011/008 ESTIMATED AFR/AP 26 JUN 020/030 PREDICTED AFR/AP 27 JUN-29 JUN 015/020-015/017-012/012
VI. Probabilidades de Actividad Geomagnética 27 JUN a 29 JUN
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 35% | 35% | 20% |
| Tormenta Menor | 20% | 20% | 10% |
| Tormenta Mayor-Severa | 05% | 05% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 40% | 40% | 25% |
| Tormenta Menor | 25% | 25% | 15% |
| Tormenta Mayor-Severa | 10% | 10% | 01% |
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