Viendo archivo del jueves, 5 marzo 1998

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 1998 Mar 05 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 064 Publicado el 2200Z a las 05 MAR 1998

IA. Análisis de regiones solares activas y de actividad desde 04-2100Z hasta 05-2100Z

SOLAR ACTIVITY WAS LOW. REGION 8171 (S24W75) CONTINUES TO PRODUCE C-CLASS FLARES. THE LARGEST OF THESE WAS A C4/SF AT 05/0912Z. REGION 8172 (N22W49) HAS GROWN INTO A SMALL C-TYPE SUNSPOT GROUP.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE LOW. C-CLASS ACTIVITY IS EXPECTED TO CONTINUE IN REGION 8171. AN M-CLASS FLARE IS POSSIBLE FROM THIS REGION BEFORE IT DEPARTS THE VISIBLE DISK.
IIA. Resumen de la actividad geofísica 04-2100Z a 05-2100Z
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS EXPECTED TO BE QUIET TO UNSETTLED.
III. Probabilidades del evento 06 MAR a 08 MAR
Clase M05%05%05%
Clase X01%01%01%
Protón01%01%01%
PCAFGREEN
IV. Penticton 10.7cm flujo
  Observado       05 MAR 097
  Previsto   06 MAR-08 MAR  094/092/090
  Media de 90 Días        05 MAR 095
V. Índices Geomagnéticos A
OBSERVED AFR/AP 04 MAR  004/008
ESTIMATED AFR/AP 05 MAR  006/008
PREDICTED AFR/AP 06 MAR-08 MAR  005/008-010/010-010/012
VI. Probabilidades de Actividad Geomagnética 06 MAR a 08 MAR
A. Latitudes Medias
Activo10%10%10%
Tormenta Menor05%05%05%
Tormenta Mayor-Severa01%05%05%
B. Latitudes Altas
Activo10%10%10%
Tormenta Menor05%05%05%
Tormenta Mayor-Severa01%05%05%

All times in UTC

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