Viendo archivo del miércoles, 23 febrero 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 Feb 23 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 054 Publicado el 2200Z a las 23 FEB 2000IA. Análisis de regiones solares activas y de actividad desde 22-2100Z hasta 23-2100Z SOLAR ACTIVITY WAS MODERATE DUE TO A SINGLE
UNCORRELATED M1 X-RAY FLARE AT 22/2147Z. THE FLARE WAS PROBABLY THE
SUPERPOSITION OF THREE EVENTS, A LONG DURATION C9 AND IMPULSIVE M1
AND C7 FLARES, BUT WITHOUT OPTICAL CORRELATION IT IS IMPOSSIBLE TO
BE SURE. THE REMAINDER OF THE PERIOD SAW NUMEROUS UNCORRELATED
C-CLASS FLARES AMIDST A BACKGROUND X-RAY FLUX AVERAGING NEARLY C2.
THREE NEW REGIONS WERE NUMBERED TODAY, 8884 (S11W74), 8885 (N11W43),
AND 8886 (S14E31).
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE
PREDOMINANTLY LOW, WITH ISOLATED M-CLASS FLARES POSSIBLE. SOLAR
ACTIVITY IS EXPECTED TO BE ON THE RISE BY THE END OF THE PERIOD.
IMAGERY FROM THE YOHKOH SOFT X-RAY TELESCOPE SUGGESTS AT LEAST TWO
LARGE ACTIVE REGIONS WILL SOON BE ROTATING ONTO THE DISK.
IIA. Resumen de la actividad geofísica 22-2100Z a 23-2100Z
THE GEOMAGNETIC FIELD WAS PREDOMINANTLY QUIET TO UNSETTLED. THE
FIELD INCREASED TO ACTIVE BETWEEN 15Z AND 18Z DUE TO THE ARRIVAL OF
A CO-ROTATING INTERACTION REGION (CIR) SEEN IN ACE DATA. THIS CIR
BROUGHT INCREASED SOLAR WIND VELOCITIES AND MAGNETIC FIELD STRENGTH;
BZ FLUCTUATED WILDLY BETWEEN -15 AND 10 NT. THE CIR HERALDS THE
EXPECTED RETURN OF A HIGH SPEED CORONAL HOLE STREAM.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE UNSETTLED TO ACTIVE IN THE MIDDLE LATITUDES AND
UNSETTLED TO MINOR STORM IN THE HIGHER LATITUDES FOR THE FIRST TWO
DAYS OF THE FORECAST PERIOD DUE TO THE EFFECTS OF A RECURRENT
CORONAL HOLE STREAM. ON THE THIRD DAY ACTIVITY IS EXPECTED TO
DIMINISH.
III. Probabilidades del evento 24 FEB a 26 FEB
| Clase M | 30% | 30% | 30% |
| Clase X | 05% | 05% | 05% |
| Protón | 01% | 01% | 01% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 23 FEB 185 Previsto 24 FEB-26 FEB 185/185/190 Media de 90 Días 23 FEB 164
V. Índices Geomagnéticos A
OBSERVED AFR/AP 22 FEB 005/005 ESTIMATED AFR/AP 23 FEB 010/012 PREDICTED AFR/AP 24 FEB-26 FEB 020/023-020/018-015/015
VI. Probabilidades de Actividad Geomagnética 24 FEB a 26 FEB
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 50% | 50% | 35% |
| Tormenta Menor | 15% | 15% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 60% | 60% | 45% |
| Tormenta Menor | 20% | 20% | 10% |
| Tormenta Mayor-Severa | 05% | 05% | 01% |
All times in UTC
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