Affichage des archives de mardi, 5 mai 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 May 05 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 125 publié à 2200Z le 05 MAY 1998

IA. Analyse des régions solaires actives et activité du 04-2100Z au 05-2100Z

SOLAR ACTIVITY HAS BEEN LOW. THE DAY'S EVENTS CONSISTED OF OCCASIONAL C-CLASS FLARES. THE LARGEST OF THESE WAS A C7.3 AT 1938Z. THE SOURCE FOR MOST OF THE ACTIVITY WAS REGION 8214 (N27W31). THIS REGION IS GROWING AND HAS BRIGHT PLAGE WITH FREQUENT FLUCTUATIONS. OBSERVERS ARE REPORTING GROWTH AND DEVELOPMENT OF PENUMBRA IN THE INTERMEDIATE SPOTS. THE CURRENT MAGNETIC CONFIGURATION IS MORE COMPLEX TODAY (BETA-GAMMA) AND THE REGION IS BECOMING COMPACT. REGION 8210 (S17W60) WAS RELATIVELY CALM TODAY, SHOWED A SLIGHT INCREASE IN AREA, BUT WAS REPORTED TO PRODUCE ONLY A FEW SUBFLARES.
IB. Prévisions d'activité solaire
SOLAR ACTIVITY IS EXPECTED TO BE MODERATE. THERE IS A GOOD CHANCE FOR AN M-CLASS EVENT FROM REGION 8214. THERE IS ALSO A POSSIBILITY FOR A MAJOR FLARE FROM THIS REGION, ESPECIALLY IF THE CURRENT TRENDS CONTINUE. REGION 8210 CONTINUES TO POSE A FAIR M-CLASS THREAT AS WELL.
IIA. Résumé de l'activité géophysique du 04-2100Z au 05-2100Z
THE GEOMAGNETIC FIELD HAS RANGED FROM UNSETTLED TO MAJOR STORM LEVELS OVER THE PAST 24 HOURS. AN INITIALLY UNSETTLED TO ACTIVE FIELD BECAME DISTURBED BETWEEN 0300-0700Z, WITH MAJOR STORM CONDITIONS OBSERVED AT MID AND HIGH LATITUDE STATIONS. FROM 0700-2100Z THE FIELD HAS BEEN CHARACTERIZED BY PREDOMINANTLY ACTIVE LEVELS, WITH SOME MINOR STORM PERIODS AT THE HIGH LATITUDE STATIONS. THE MAJOR GEOMAGNETIC STORM THAT BEGAN WITH THE SSC OF 04/0300Z OFFICIALLY ENDED AT 05/0900UT. THE CURRENT ACTIVITY IS ASSOCIATED WITH THE X1/3B/HALO CME EVENT OF 02/1342Z. THIS EVENT WAS INITIALLY SEEN AT ACE AS A STRONG SHOCK AT 04/0229Z FOLLOWED BY A PERIOD OF NEGATIVE BZ FROM 04/0230-0430Z. THE SOLAR WIND DATA HAVE CONTINUED TO SHOW CHARACTERISTICS OF TRANSIENT FLOW OVER THE PAST 24 HOURS, NAMELY STRONG MAGNETIC FIELDS, VARIABLE TEMPERATURES, AND VARIABLE BUT HIGH VELOCITIES. THE FLOW DOES NOT SHOW THE 'CLASSIC CLOUD' STRUCTURE, SUGGESTING THAT THE DRIVER MISSED HITTING THE EARTH DIRECTLY. THE GREATER THAN 2 MEV ELECTRONS EXCEEDED HIGH LEVELS DURING THE PAST 24 HOURS.
IIB. Prévision de l'activité géophysique
THE GEOMAGNETIC FIELD IS EXPECTED TO BE PREDOMINANTLY ACTIVE FOR THE NEXT 24-36 HOURS DUE TO LINGERING EFFECTS OF THE CURRENT DISTURBANCE. CONDITIONS SHOULD RETURN TO UNSETTLED TO QUIET THEREAFTER.
III. Probabilité d'éruption solaire du 06 MAY au 08 MAY
Classe M75%75%75%
Classe X20%20%20%
Proton20%20%20%
PCAFYELLOW
IV. Flux Penticton 10.7 cm
  Observé       05 MAY 133
  Prévisionnel   06 MAY-08 MAY  135/135/130
  Moyenne des 90 derniers jours        05 MAY 106
V. Indice géomagnetique A
OBSERVED AFR/AP 04 MAY  090/096
ESTIMATED AFR/AP 05 MAY  025/035
PREDICTED AFR/AP 06 MAY-08 MAY  020/025-015/020-005/013
VI. Probabilités d'activité géomagnétique du 06 MAY au 08 MAY
A. Latitudes moyennes
Actif20%20%10%
Tempête mineure10%05%05%
Tempête majeure/sévère10%05%05%
B. Hautes latitudes
Actif25%25%10%
Tempête mineure10%05%05%
Tempête majeure/sévère10%05%05%

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