Viendo archivo del martes, 25 marzo 1997

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 1997 Mar 25 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 084 Publicado el 2200Z a las 25 MAR 1997

IA. Análisis de regiones solares activas y de actividad desde 24-2100Z hasta 25-2100Z

THE DISK REMAINED SPOTLESS AND SOLAR ACTIVITY CONTINUED AT A VERY LOW LEVEL.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY SHOULD CONTINUE AT A VERY LOW LEVEL FOR THE NEXT THREE DAYS.
IIA. Resumen de la actividad geofísica 24-2100Z a 25-2100Z
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED. RECENT SOLAR WIND DATA INDICATE THAT THE EXPECTED CORONAL HOLE RELATED STREAM HAS NOT YET REACHED EARTH.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS FORECAST TO BE GENERALLY UNSETTLED TO ACTIVE ON 26-27 MAR. ISOLATED MINOR STORM CONDITIONS ARE POSSIBLE DURING THAT PERIOD. QUIET TO UNSETTLED LEVELS ARE EXPECTED TO RETURN ON 28 MAR.
III. Probabilidades del evento 26 MAR a 28 MAR
Clase M01%01%01%
Clase X01%01%01%
Protón01%01%01%
PCAFGREEN
IV. Penticton 10.7cm flujo
  Observado       25 MAR 071
  Previsto   26 MAR-28 MAR  071/071/071
  Media de 90 Días        25 MAR 074
V. Índices Geomagnéticos A
OBSERVED AFR/AP 24 MAR  008/006
ESTIMATED AFR/AP 25 MAR  011/008
PREDICTED AFR/AP 26 MAR-28 MAR  015/015-020/020-010/010
VI. Probabilidades de Actividad Geomagnética 26 MAR a 28 MAR
A. Latitudes Medias
Activo25%30%15%
Tormenta Menor15%15%10%
Tormenta Mayor-Severa05%05%01%
B. Latitudes Altas
Activo25%35%20%
Tormenta Menor15%10%10%
Tormenta Mayor-Severa05%05%05%

All times in UTC

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