Vaata kolmapäev, 6 september 2000 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 2000 Sep 06 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 250 Välja antud 2200Z kuni 06 SEP 2000

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 05-2100Z kuni 06-2100Z

SOLAR ACTIVITY CONTINUED AT LOW LEVELS. REGION 9154 (S18W21) REMAINED MODERATE IN SIZE AND MAGNETIC COMPLEXITY AND PRODUCED OCCASIONAL C-CLASS SUBFLARES. REGION 9149 (N13W49) ALSO REMAINED MODERATE IN SIZE AND COMPLEXITY, BUT PRODUCED NO FLARES. THE REMAINING REGIONS WERE SIMPLE AND STABLE. NEW REGIONS 9156 (S27E49) AND 9157 (N21E63) WERE NUMBERED.
IB. Päikese aktiivsuse ennustus
LOW TO MODERATE ACTIVITY IS EXPECTED. REGIONS 9154 AND 9149 COULD PRODUCE ISOLATED M-CLASS FLARES. IIA. GEOPHYSICAL ACTIVITY SUMMARY 05/2100Z TO 06/2100Z: GEOMAGNETIC FIELD ACTIVITY WAS AT QUIET TO UNSETTLED LEVELS UNTIL ABOUT 06/1700 UTC. ACE REAL TIME SOLAR WIND MEASUREMENTS INDICATED AN INTERPLANETARY SHOCK PASSAGE AT L1 AT ABOUT 06/1614 UTC FOLLOWED BY A SUDDEN IMPULSE AT 06/1704 UTC (16 NT, AS MEASURED BY THE BOULDER USGS MAGNETOMETER). FIELD ACTIVITY INCREASED TO UNSETTLED TO ACTIVE LEVELS FOLLOWING THE IMPULSE. THIS ACTIVITY IS LIKELY ASSOCIATED WITH A LARGE FILAMENT DISAPPEARANCE/PARTIAL-HALO CME OBSERVED ON 4 SEPTEMBER. THE GREATER THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT MAY REACH MODERATE TO HIGH LEVELS DURING THE LATTER HALF OF THE PERIOD.
IIB. Geofüüsikalise aktiivsuse ennustus
GEOMAGNETIC FIELD ACTIVITY IS EXPECTED TO BE AT UNSETTLED TO MINOR STORM LEVELS DURING THE FIRST HALF OF THE PERIOD AS THE CME-RELATED DISTURBANCE CONTINUES. FIELD ACTIVITY IS EXPECTED TO DECREASE TO UNSETTLED LEVELS DURING THE LATTER HALF OF THE PERIOD AS THE DISTURBANCE SUBSIDES.
III. Sündmuste tõenäosus 07 SEPkuni 09 SEP
Klass M30%30%30%
Klass X05%05%05%
Prooton05%05%05%
PCAFGREEN
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       06 SEP 179
  Prognoositud   07 SEP-09 SEP  185/190/190
  90 päeva keskmine        06 SEP 181
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 05 SEP  008/008
ESTIMATED AFR/AP 06 SEP  010/010
PREDICTED AFR/AP 07 SEP-09 SEP  030/030-020/020-015/015
VI. Geomagnetilised aktiivsuse tõenäosused 07 SEP kuni 09 SEP
A. Keskmistel laiuskraadidel
Aktiivne20%30%25%
Väike torm30%20%10%
Suur-tõsine torm15%10%05%
B. Kõrgetel laiuskraadidel
Aktiivne25%35%30%
Väike torm35%25%15%
Suur-tõsine torm20%15%10%

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