Affichage des archives de samedi, 13 juin 1998

Rapport d'activité solaire

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.
Rapport d'activité solaire et géophysique 1998 Jun 13 2200 UTC
Fait par le NOAA © SWPC et adapté par SpaceWeatherLive.com

Rapport de l'USAF/NOAA sur l'activité solaire et géophysique

SDF numéro 164 publié à 2200Z le 13 JUN 1998

IA. Analyse des régions solaires actives et activité du 12-2100Z au 13-2100Z

SOLAR ACTIVITY WAS MODERATE DUE TO AN M1 X-RAY EVENT AT 0420Z. AN EXAMINATION OF GOES X-RAY DATA SHOWED THAT THIS LEVEL RESULTED FROM THE SUPERPOSITION OF A SHORT, IMPULSIVE 1N FLARE FROM REGION 8242 (S23E42) ON TOP OF A LONG DURATION X-RAY EVENT. THE LONG DURATION EVENT BEGAN AT ABOUT 03Z AND CONTINUED THROUGH ABOUT 08Z. DURING THIS SAME INTERVAL A SERIES OF LASCO IMAGES (STARTING AT 0355 AND ENDING AT 0730Z) SHOWED TRANSIENT MATERIAL MOVING OFF OF THE WEST LIMB. REGION 8242 PRODUCED ADDITIONAL C-CLASS SUBFLARES DURING THE DAY. REGION 8237 (S24W08) PRODUCED A C-CLASS EVENT AT 1554Z WHICH WAS ACCOMPANIED BY PARALLEL H-ALPHA FLARE RIBBONS. NEW REGION 8245 (S19E15) EMERGED ON THE DISK AND SHOWED STEADY GROWTH. NEW REGION 8246 WAS ASSIGNED TO THE SPOTS THAT EMERGED NEAR N14W48, JUST EAST OF REGION 8234 (N16W57). REGION 8240 HAS NOW ROTATED BEYOND THE WEST LIMB.
IB. Prévisions d'activité solaire
SOLAR ACTIVITY IS EXPECTED TO BE PREDOMINANTLY LOW. THERE IS A SLIGHT CHANCE FOR AN ISOLATED M-CLASS EVENT, WITH REGION 8242 AS THE MOST LIKELY SOURCE.
IIA. Résumé de l'activité géophysique du 12-2100Z au 13-2100Z
THE GEOMAGNETIC FIELD WAS QUIET FROM THE BEGINNING OF THE PERIOD THROUGH 1927Z WHEN A WEAK (BUT NOT SUDDEN) IMPULSE WAS OBSERVED ON THE DAYSIDE MAGNETOMETERS. THE IMPULSE WAS PRECEDED BY COMPRESSION SIGNATURE AT ACE AT 1855Z. THE L1 DATA SHOWED MANY FEATURES SIMILAR TO A SHOCK (ENHANCED VELOCITY, DENSITY, TEMPERATURE AND MAGNETIC FIELDS), BUT CHANGED OVER A LONGER TIME INTERVAL THAN A TRUE SHOCK (ABOUT 5 MINUTES), SUGGESTING THAT L1 WAS EITHER ON THE FLANKS OF A FAST CME OR WAS AHEAD OF A RELATIVELY SLOW CME. THE FORMER SEEMS MORE LIKELY, GIVEN THE CLEAR OBSERVATIONS OF TRANSIENT ACVITITY FROM THE EAST LIMB ON THE 11TH. THE GEOMAGNETIC ACTIVITY LEVELS RESPONDED MILDLY BY INCREASING FROM QUIET TO UNSETTLED LEVELS FOR THE REMAINDER OF THE PERIOD.
IIB. Prévision de l'activité géophysique
THE GEOMAGNETIC FIELD IS EXPECTED TO BE GENERALLY UNSETTLED FOR THE NEXT 24 HOURS. QUIET TO UNSETTLED LEVELS ARE EXPECTED TO PREDOMINATE FOR THE SECOND AND THIRD DAYS.
III. Probabilité d'éruption solaire du 14 JUN au 16 JUN
Classe M20%20%20%
Classe X01%01%01%
Proton01%01%01%
PCAFGREEN
IV. Flux Penticton 10.7 cm
  Observé       13 JUN 111
  Prévisionnel   14 JUN-16 JUN  110/105/105
  Moyenne des 90 derniers jours        13 JUN 110
V. Indice géomagnetique A
OBSERVED AFR/AP 12 JUN  006/008
ESTIMATED AFR/AP 13 JUN  005/005
PREDICTED AFR/AP 14 JUN-16 JUN  005/010-005/010-005/010
VI. Probabilités d'activité géomagnétique du 14 JUN au 16 JUN
A. Latitudes moyennes
Actif10%10%10%
Tempête mineure05%05%05%
Tempête majeure/sévère01%01%01%
B. Hautes latitudes
Actif10%10%10%
Tempête mineure05%05%05%
Tempête majeure/sévère01%01%01%

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