Viendo archivo del viernes, 23 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 23 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 175 Publicado el 2200Z a las 23 JUN 2000IA. Análisis de regiones solares activas y de actividad desde 22-2100Z hasta 23-2100Z SOLAR ACTIVITY INCREASED TO MODERATE LEVELS. REGION
9046 (N21W34) PRODUCED AN M2/2B FLARE AT 23/0407Z ASSOCIATED WITH A
240 SFU TENFLARE, AND TYPE II AND IV RADIO SWEEPS. REGION 9042
(N23W72) PRODUCED AN M3/1F FLARE AT 23/1431Z ASSOCIATED WITH A 250
SFU TENFLARE, TYPE II AND IV RADIO SWEEPS, AND A PARTIAL-HALO CME.
BOTH REGIONS SHOWED GRADUAL DECAY, BUT RETAINED MIXED-POLARITY
MAGNETIC STRUCTURES. THE REMAINING REGIONS WERE STABLE AND SIMPLY
STRUCTURED, INCLUDING NEWLY NUMBERED REGIONS 9058 (S14W15) AND 9059
(N14E30).
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE AT
LOW TO MODERATE LEVELS. REGIONS 9042 AND 9046 MAY PRODUCE ISOLATED
M-CLASS FLARES.
IIA. Resumen de la actividad geofísica 22-2100Z a 23-2100Z
GEOMAGNETIC FIELD ACTIVITY RANGED FROM QUIET TO MINOR STORM LEVELS. A
SUDDEN IMPULSE (SI) OCCURRED AT 23/1305Z WITH A MAGNITUDE OF 29
NANOTESLA (AS MEASURED BY THE BOULDER USGS MAGNETOMETER). ACTIVITY
INCREASED TO UNSETTLED TO MINOR STORM LEVELS FOLLOWING THE SI. A
PROTON ENHANCEMENT AT GREATER THAN 10 MEV BEGAN AT GEOSYNCHRONOUS
ORBIT AROUND 23/1600Z. THE ENHANCEMENT FOLLOWED THE M3/1F FROM
REGION 9042.
IIB. Pronóstico de la actividad geofísica
GEOMAGNETIC FIELD ACTIVITY IS
EXPECTED TO REMAIN AT UNSETTLED TO MINOR STORM LEVELS THROUGH MOST
OF THE PERIOD. THE GREATER THAN 10 MEV PROTON FLUX AT GEOSYNCHRONOUS
ORBIT IS EXPECTED TO RETURN TO BACKGROUND LEVELS EARLY IN THE
PERIOD. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT
IS EXPECTED TO RISE TO MODERATE TO HIGH LEVELS LATE IN THE PERIOD.
III. Probabilidades del evento 24 JUN a 26 JUN
| Clase M | 40% | 40% | 35% |
| Clase X | 10% | 10% | 05% |
| Protón | 10% | 10% | 05% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 23 JUN 175 Previsto 24 JUN-26 JUN 175/170/165 Media de 90 Días 23 JUN 186
V. Índices Geomagnéticos A
OBSERVED AFR/AP 22 JUN 011/008 ESTIMATED AFR/AP 23 JUN 018/015 PREDICTED AFR/AP 24 JUN-26 JUN 020/025-020/025-020/025
VI. Probabilidades de Actividad Geomagnética 24 JUN a 26 JUN
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 40% | 40% | 40% |
| Tormenta Menor | 15% | 15% | 15% |
| Tormenta Mayor-Severa | 05% | 05% | 05% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 40% | 40% | 40% |
| Tormenta Menor | 20% | 20% | 20% |
| Tormenta Mayor-Severa | 05% | 05% | 05% |
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