Vaata neljapäev, 23 august 2001 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 2001 Aug 23 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 235 Välja antud 2200Z kuni 23 Aug 2001

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 22-2100Z kuni 23-2100Z

Solar activity decreased to low levels. Region 9591 (S17E53) produced frequent, impulsive mid-level C-class flares with minor radio emission. This region showed a magnetic delta structure in its trailing sunspots and a weak delta in its interior spots. Currently, Region 9591 spans about 30 degrees in longitude. However, it appeared likely this region was comprised of two abutted sunspot groups, which may be split into separate groups once this complex rotates further into view. Minor polarity mixing was evident in Regions 9582 (N28W33) and 9585 (N14W16), but both regions were inactive as they showed signs of decay. The remaining active regions were unremarkable. New Region 9593 (N00E01) was numbered.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be moderate with a good chance for an isolated M-class flare from Region 9591. There is also a slight chance for a major flare from this region.
IIA. Summaarne geofüüsikaline aktiivsus 22-2100Z kuni 23-2100Z
Geomagnetic field activity decreased to quiet to unsettled levels as coronal hole effects subsided.
IIB. Geofüüsikalise aktiivsuse ennustus
Geomagnetic field activity is expected to be at quiet to unsettled levels during the first half of the period increasing to unsettled to active levels during the rest of the period. There will be a slight chance for a proton event during the period. The greater than 2 MeV electron flux at geosynchronous orbit may reach high levels during the first half of the forecast period.
III. Sündmuste tõenäosus 24 Augkuni 26 Aug
Klass M50%50%50%
Klass X10%10%10%
Prooton05%10%10%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       23 Aug 170
  Prognoositud   24 Aug-26 Aug  175/180/180
  90 päeva keskmine        23 Aug 152
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 22 Aug  014/017
  Hinnanguline     Afr/Ap 23 Aug  009/010
  Prognoositud    Afr/Ap 24 Aug-26 Aug  010/010-012/012-015/012
VI. Geomagnetilised aktiivsuse tõenäosused 24 Aug kuni 26 Aug
A. Keskmistel laiuskraadidel
Aktiivne20%25%30%
Väike torm05%10%15%
Suur-tõsine torm01%01%05%
B. Kõrgetel laiuskraadidel
Aktiivne25%30%35%
Väike torm10%15%20%
Suur-tõsine torm01%01%10%

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