Vaata laupäev, 3 jaanuar 1998 arhiivi

Päikese aktiivsuse aruanne

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.
Päikese ja geofüüsikalise aktiivsuse aruanne 1998 Jan 03 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 003 Välja antud 2200Z kuni 03 JAN 1998

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 02-2100Z kuni 03-2100Z

SOLAR ACTIVITY CONTINUED AT A MODERATE LEVEL DUE TO AN OPTICALLY UNCORRELATED M2 AT 03/1719Z. THE LIKELY SOURCE FOR THIS EVENT WAS REGION 8124 LOCATED ONE DAY BEHIND THE WEST LIMB AT S22. TWO LARGE CORONAL MASS EJECTIONS OCCURRED. THE FIRST WAS COINCIDENT WITH A LONG DURATION (02/2335-03/0630Z) B6 X-RAY ENHANCEMENT. THE CME WAS NEARLY A COMPLETE HALO. THE SOURCE OF THIS CME WAS THE SLOW DISSOLUTION OF FILAMENT MATERIAL LOCATED NEAR N47W03. A POST-ERUPTION ARCADE BECAME VISIBLE DOWN TO NEAR REGION 8126 (N21W61). THE SECOND CME OCCURRED NEAR 03/1000Z FROM HIGH LATITUDES IN THE NORTHWEST QUADRANT. THIS EVENT WAS VERY BRIGHT IN CORONAGRAPH IMAGERY AND LIKELY RELATED TO THE ERUPTION OF LARGE POLAR CROWN FILAMENTS NEAR THE NORTHWEST LIMB. THE TRAJECTORY OF THIS MATERIAL WAS HIGHLY INCLINED TO THE ECLIPTIC.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY SHOULD BECOME VERY LOW TO LOW FOR THE NEXT THREE DAYS AS REGION 8124 MOVES SEVERAL DAYS BEHIND THE WEST LIMB.
IIA. Summaarne geofüüsikaline aktiivsus 02-2100Z kuni 03-2100Z
THE GEOMAGNETIC FIELD WAS PREDOMINANTLY QUIET.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD SHOULD BE QUIET TO SLIGHTLY UNSETTLED FOR 04-05 JAN. UNSETTLED TO ACTIVE CONDITIONS ARE FORECAST IN THE LATTER HALF OF 06 JAN AND FOR 07 JAN IN RESPONSE TO THE HALO EVENT MENTIONED ABOVE. ISOLATED MINOR STORM CONDITIONS AT HIGH LATITUDES ARE POSSIBLE DURING THE DISTURBANCE. THE SECOND CORONAL MASS EJECTION IS NOT EXPECTED TO IMPACT THE EARTH.
III. Sündmuste tõenäosus 04 JANkuni 06 JAN
Klass M05%05%01%
Klass X01%01%01%
Prooton01%01%01%
PCAFGREEN
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       03 JAN 101
  Prognoositud   04 JAN-06 JAN  092/088/086
  90 päeva keskmine        03 JAN 095
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 02 JAN  006/004
ESTIMATED AFR/AP 03 JAN  005/005
PREDICTED AFR/AP 04 JAN-06 JAN  005/005-005/005-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 04 JAN kuni 06 JAN
A. Keskmistel laiuskraadidel
Aktiivne10%10%35%
Väike torm05%05%15%
Suur-tõsine torm01%01%05%
B. Kõrgetel laiuskraadidel
Aktiivne10%10%40%
Väike torm05%05%25%
Suur-tõsine torm01%01%10%

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