Vaata laupäev, 29 august 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 Aug 29 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 241 Välja antud 2200Z kuni 29 AUG 1998

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 28-2100Z kuni 29-2100Z

SOLAR ACTIVITY WAS LOW. SEVERAL C-CLASS EVENTS WERE OBSERVED DURING THE LAST 24 HOURS. THE LARGEST OF THESE WAS A C5 AT 1836Z WHICH WAS NOT OBSERVED OPTICALLY. REGION 8307 (N32W52) CONTRIBUTED AT LEAST ONE OF THE C-CLASS EVENTS AT 1535Z. THE GROUP WAS ESSENTIALLY UNCHANGED AND STABLE OVER THE PAST 24 HOURS. REGION 8319 (N19W29) PRODUCED A FEW SUBFLARES DURING THE PERIOD AND CONTINUES TO INCREASE IN SIZE. REGION 8323 (S23E65) ROTATED FURTHER INTO VIEW TODAY AND APPEARS TO BE A BIPOLAR GROUP WITH PENUMBRA IN THE LEADER AND TRAILER.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY IS EXPECTED TO BE PREDOMINANTLY LOW. HOWEVER, EACH OF THE REGIONS 8307, 8319 AND 8323 HAS THE POTENTIAL FOR AN M-CLASS EVENT, SO THERE IS A SLIGHT CHANCE FOR MODERATE LEVELS DURING THE NEXT THREE DAYS.
IIA. Summaarne geofüüsikaline aktiivsus 28-2100Z kuni 29-2100Z
THE GEOMAGNETIC FIELD WAS MOSTLY UNSETTLED TO ACTIVE. THERE WERE SOME ISOLATED MINOR STORM PERIODS AT THE HIGH LATITUDES. ACE REAL-TIME SOLAR WIND DATA CONTINUE TO SHOW A LOW DENSITY, HIGH SPEED STREAM WITH WAVE-LIKE ACTIVITY IN THE BZ INTERPLANETARY FIELD. VARIATIONS IN BZ DOWN TO -5 NT ARE UNDOUBTEDLY THE SOURCE OF THE ENHANCED MAGNETIC ACTIVITY. THE GREATER THAN 2 MEV ELECTRON FLUXES HAVE BEEN HIGH. THE GREATER THAN 10 MEV PROTON EVENT THAT BEGAN 24/2355Z ENDED TODAY AT 29/1210Z.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS EXPECTED TO BE UNSETTLED TO ACTIVE FOR THE NEXT TWO DAYS, DECLINING TO UNSETTLED TO SLIGHTLY ACTIVE BY THE THIRD DAY.
III. Sündmuste tõenäosus 30 AUGkuni 01 SEP
Klass M20%20%20%
Klass X10%10%10%
Prooton15%15%15%
PCAFGREEN
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       29 AUG 147
  Prognoositud   30 AUG-01 SEP  150/150/140
  90 päeva keskmine        29 AUG 118
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 28 AUG  026/025
ESTIMATED AFR/AP 29 AUG  015/020
PREDICTED AFR/AP 30 AUG-01 SEP  015/015-015/015-010/015
VI. Geomagnetilised aktiivsuse tõenäosused 30 AUG kuni 01 SEP
A. Keskmistel laiuskraadidel
Aktiivne40%40%20%
Väike torm10%05%05%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne50%40%35%
Väike torm20%15%10%
Suur-tõsine torm05%05%05%

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