Affichage des archives de lundi, 28 juin 1999

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 1999 Jun 28 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 179 publié à 2200Z le 28 JUN 1999

IA. Analyse des régions solaires actives et activité du 27-2100Z au 28-2100Z

SOLAR ACTIVITY WAS LOW. REGION 8611 (S25E47) WAS THE MOST ACTIVE REGION ON THE DISK TODAY AND PRODUCED NUMEROUS C-CLASS SUBFLARES. THE LARGEST OF THESE WAS A C6/1F AT 1934Z. THIS GROUP EXHIBITED VERY BRIGHT PLAGE ALL DAY AND IS GROWING STEADILY. REGION 8598 (N22W25) IS STILL THE LARGEST SUNSPOT GROUP ON THE DISK BUT COULD ONLY MUSTER ONE SUBFLARE, IN SPITE OF A DELTA SPOT NEAR REGION CENTER. THIS GROUP SHOWED SIGNIFICANT DECAY OF MAGNETIC FLUX AND IS CLEARLY ON THE DECLINE. A PARTIAL HALO CME WAS REPORTED BY LASCO THAT WAS ASSOCIATED WITH A SIGNATURE IN EIT IN THE NORTHWEST QUADRANT OF THE SOLAR DISK. THESE EVENTS WERE ALSO TIME COINCIDENT WITH YESTERDAY'S M1 FLARE FROM REGION 8592 AT N23W25.
IB. Prévisions d'activité solaire
SOLAR ACTIVITY IS EXPECTED TO BE LOW TO MODERATE. REGIONS 8598 AND 8611 ARE THE BEST CANDIDATES FOR PRODUCING AN ISOLATED M-CLASS EVENT OVER THE NEXT THREE DAYS. REGIONS 8602 (N18E08), AND 8603 (S15E18) MIGHT ALSO CONTRIBUTE, GIVEN THE CURRENT SLOW GROWTH TREND IN THESE REGIONS.
IIA. Résumé de l'activité géophysique du 27-2100Z au 28-2100Z
THE GEOMAGNETIC FIELD RANGED FROM QUIET TO MAJOR STORM LEVELS. YESTERDAY'S ACTIVE CONDITIONS DECLINED TO QUIET AROUND 28/0000Z. AROUND 28/0400Z THE SOLAR WIND VELOCITY BEGAN TO INCREASE SIGNIFICANTLY, REACHING SPEEDS AS HIGH AS 900 KM/S BY 0510Z. THE GEOMAGNETIC FIELD RESPONDED WITH A PERIOD OF MAJOR STORM FROM 0300-0600Z, FOLLOWED BY AN ACTIVE TO MINOR STORM PERIOD FROM 0600-0900Z. THE INTERPLANETARY MAGNETIC FIELD SHOWED SOME MILDLY NEGATIVE BZ FROM 0400-0600Z BUT RETURNED TO NOMINAL LEVELS THEREAFTER. IN RESPONSE THE GEOMAGNETIC FIELD ALSO CALMED TO QUIET TO UNSETTLED FROM 0900Z THROUGH THE END OF THE DAY. GIVEN THE HIGH SPEED AND VERY LOW DENSITY SEEN WITH THIS SOLAR WIND EVENT, IT IS MOST LIKELY THAT ACE OBSERVED THE RAREFACTION REGION BEHIND THE PARTIAL HALO CME OF 24 JUNE, WHICH WAS KNOWN TO BE DIRECTED SLIGHTLY TO THE WEST OF THE SUN-EARTH LINE.
IIB. Prévision de l'activité géophysique
THE GEOMAGNETIC FIELD IS EXPECTED TO BE UNSETTLED TO ACTIVE FOR THE NEXT 24 HOURS. MOSTLY UNSETTLED CONDITIONS SHOULD DOMINATE ON THE SECOND DAY. PREDOMINANTLY UNSETTLED LEVELS ARE ALSO EXPECTED ON THE THIRD DAY, BUT THERE WILL BE AN ENHANCED PROBABILITY FOR SOME ACTIVE PERIODS BECAUSE OF THE PARTIAL HALO CME OF THE 27TH.
III. Probabilité d'éruption solaire du 29 JUN au 01 JUL
Classe M55%50%45%
Classe X05%05%05%
Proton10%10%05%
PCAFGREEN
IV. Flux Penticton 10.7 cm
  Observé       28 JUN 197
  Prévisionnel   29 JUN-01 JUL  180/175/170
  Moyenne des 90 derniers jours        28 JUN 144
V. Indice géomagnetique A
OBSERVED AFR/AP 27 JUN  015/021
ESTIMATED AFR/AP 28 JUN  020/025
PREDICTED AFR/AP 29 JUN-01 JUL  012/018-010/012-012/015
VI. Probabilités d'activité géomagnétique du 29 JUN au 01 JUL
A. Latitudes moyennes
Actif25%15%20%
Tempête mineure05%05%10%
Tempête majeure/sévère05%01%05%
B. Hautes latitudes
Actif25%15%20%
Tempête mineure05%05%15%
Tempête majeure/sévère05%01%05%

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