Viendo archivo del lunes, 1 marzo 1999

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 1999 Mar 01 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 060 Publicado el 2200Z a las 01 MAR 1999

IA. Análisis de regiones solares activas y de actividad desde 28-2100Z hasta 01-2100Z

SOLAR ACTIVITY RETURNED TO LOW LEVELS. REGION 8471 (N28W26) PRODUCED SEVERAL LOW LEVEL C-CLASS SUBFLARES. ON 28 FEB, PRIOR TO THE M6/2B, THIS REGION DEVELOPED A DELTA MAGNETIC CLASSIFICATION OF MODERATE STRENGTH. IN THE INTERIM, THIS DELTA FADED AND OVERALL THE REGION DECAYED SLIGHTLY IN PENUMBRAL COVERAGE. THE MAIN NEUTRAL LINE IN THIS REGION WAS ALMOST LINEAR SUGGESTING MAGNETIC SHEAR AT THAT LOCATION, BUT VECTOR MAGNETOGRAPH DATA WERE NOT AVAILABLE TO CONFIRM THIS SUPPOSITION. REGION 8475 (N32E16) EXHIBITED GROWTH AND PRODUCED SEVERAL SUBFLARES. A DELTA MAGNETIC CONFIGURATION MAY BE FORMING IN THIS REGION. TWO SMALL AREAS OF PLAGE AND SPOTS EMERGED NEAR S15W07. THERE WERE NUMBERED AS NEW REGION 8478. THIS AREA MAY BE SPLIT INTO TWO SEPARATE REGIONS IN THE NEAR FUTURE.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY SHOULD BECOME LOW TO MODERATE. REGION 8471 REMAINS CAPABLE OF PRODUCING AN ISOLATED M-CLASS EVENT BUT FLARE FREQUENCY SHOULD DECREASE AS DECAY CONTINUES. REGION 8475 SHOULD BEGIN TO PRODUCE FREQUENT C-CLASS EVENTS AND ISOLATED M-CLASS EVENTS SHOULD GROWTH AND INCREASING MAGNETIC COMPLEXITY CONTINUE.
IIA. Resumen de la actividad geofísica 28-2100Z a 01-2100Z
THE GEOMAGNETIC FIELD RANGED FROM UNSETTLED TO MINOR STORM LEVELS. THE MOST DISTURBED PERIODS WERE 01/0000-0600Z AND 01/1200-1800Z. SOLAR WIND DATA SHOWED A LOW SPEED, HIGH DENSITY FLOW WITH NORTHWARD BZ DURING THE DISTURBANCE. IT IS POSSIBLE THIS DISTURBANCE WAS RELATED TO A FILAMENT DISRUPTION IN THE SOUTHEAST QUADRANT ON 24-25 FEB. AT THE END OF THE PERIOD, SOLAR WIND VELOCITY WAS INCREASING AND DENSITY WAS DECREASING.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD SHOULD BE PREDOMINANTLY QUIET TO UNSETTLED FOR THE NEXT THREE DAYS. ISOLATED ACTIVE CONDITIONS ARE POSSIBLE DURING THAT TIME. A SMALL CORONAL HOLE SHOULD BEGIN TO AFFECT THE EARTH'S FIELD ON 02-03 MAR.
III. Probabilidades del evento 02 MAR a 04 MAR
Clase M50%40%40%
Clase X10%10%10%
Protón05%05%05%
PCAFGREEN
IV. Penticton 10.7cm flujo
  Observado       01 MAR 120
  Previsto   02 MAR-04 MAR  120/120/118
  Media de 90 Días        01 MAR 144
V. Índices Geomagnéticos A
OBSERVED AFR/AP 28 FEB  010/014
ESTIMATED AFR/AP 01 MAR  024/025
PREDICTED AFR/AP 02 MAR-04 MAR  015/015-012/012-012/010
VI. Probabilidades de Actividad Geomagnética 02 MAR a 04 MAR
A. Latitudes Medias
Activo20%20%20%
Tormenta Menor10%10%10%
Tormenta Mayor-Severa05%05%05%
B. Latitudes Altas
Activo25%20%20%
Tormenta Menor10%10%10%
Tormenta Mayor-Severa05%05%05%

All times in UTC

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