Viendo archivo del jueves, 22 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 22 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 174 Publicado el 2200Z a las 22 JUN 2000IA. Análisis de regiones solares activas y de actividad desde 21-2100Z hasta 22-2100Z SOLAR ACTIVITY HAS BEEN LOW. REGION 9042 (N23W54)
PRODUCED MOST OF TODAY'S C-CLASS EVENTS, INCLUDES THE LARGEST, A
C5/SF AT 0023Z. REGIONS 9040 (N18W73) AND 9046 (N20W21) ALSO
EXHIBITED SUBFLARE LEVEL BRIGHTENINGS DURING THE EVENT REGION 9042
HAS CONTINUED TO DECAY, ESPECIALLY IN THE TRAILER PORTION OF THE
GROUP. REGION 9046 (N20W21) ALSO CONTRIBUTED A FEW C-CLASS EVENTS
AND HAS SHOWN A SLIGHT DECREASE IN AREA. NEW REGION 9057 (N14E72)
ROTATED INTO VIEW TODAY AS A SIMPLE H-TYPE REGION.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE
MOSTLY LOW, BUT THERE IS A CHANCE FOR AN ISOLATED M-CLASS EVENT
SOMETIME DURING THE NEXT THREE DAYS. REGIONS 9042 AND 9046 ARE
CONSIDERED TO BE THE MOST LIKELY SOURCES FOR M-CLASS FLARES.
IIA. Resumen de la actividad geofísica 21-2100Z a 22-2100Z
THE GEOMAGNETIC FIELD RANGED FROM QUIET TO ACTIVE. QUIET TO UNSETTLED
LEVELS PREDOMINATED FOR MOST OF THE DAY, BUT THERE WAS ONE ACTIVE
PERIOD FROM 0000-0300Z. REAL-TIME SOLAR WIND OBSERVATIONS FROM THE
ACE SPACECRAFT INDICATED A SOLAR SECTOR BOUNDARY CROSSING FROM AN
'AWAY' (POSITIVE) CONFIGURATION TO A 'TOWARDS' (NEGATIVE)
CONFIGURATION BETWEEN 0100-1200Z.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE MOST UNSETTLED TOMORROW, BUT GRADUAL INCREASE TO
UNSETTLED TO ACTIVE IS ANTICIPATED LATE TOMORROW OR BY THE SECOND
DAY. THE INCREASE IS EXPECTED AS A RESPONSE TO THE INFLUENCE OF A
RECURRENT CORONAL HOLE.
III. Probabilidades del evento 23 JUN a 25 JUN
| Clase M | 35% | 35% | 35% |
| Clase X | 05% | 05% | 05% |
| Protón | 05% | 05% | 05% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 22 JUN 180 Previsto 23 JUN-25 JUN 175/175/170 Media de 90 Días 22 JUN 186
V. Índices Geomagnéticos A
OBSERVED AFR/AP 21 JUN 006/008 ESTIMATED AFR/AP 22 JUN 012/012 PREDICTED AFR/AP 23 JUN-25 JUN 012/015-015/015-015/020
VI. Probabilidades de Actividad Geomagnética 23 JUN a 25 JUN
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 30% | 35% | 35% |
| Tormenta Menor | 10% | 15% | 15% |
| Tormenta Mayor-Severa | 05% | 05% | 05% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 35% | 40% | 40% |
| Tormenta Menor | 15% | 20% | 20% |
| Tormenta Mayor-Severa | 05% | 10% | 10% |
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