Vaata laupäev, 19 jaanuar 2002 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 2002 Jan 19 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 019 Välja antud 2200Z kuni 19 Jan 2002

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 18-2100Z kuni 19-2100Z

Solar activity increased to moderate levels. Region 9787 (S07E59) produced an impulsive M1/Sf flare at 19/1005 UTC with minor radio emission. Minor growth occurred in this region, but it remained simply structured. Minor growth also occurred in Regions 9786 (S25W32) and 9788 (N17E40), but both remained simple bipoles. Region 9788 produced a low-level C-class flare late in the period. Region 9782 showed a minor decrease in area and continued to display minor polarity mixing within its southern leader spots. A large filament disappeared from the northeast quadrant late on 18 January. SOHO EIT/LASCO images showed that the filament gradually disappeared and was followed by a relatively slow, non-Earth directed CME. New Regions 9789 (N15W02) and 9790 (N28E25) were numbered.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low to moderate. There will be a chance for an isolated low-level M-class flare during the period.
IIA. Summaarne geofüüsikaline aktiivsus 18-2100Z kuni 19-2100Z
Geomagnetic field activity ranged from quiet to minor storm levels. Activity increased to unsettled to minor storm levels during 19/1200 - 1800 UTC, then decreased to mostly unsettled levels. The increased activity was likely due to coronal hole effects.
IIB. Geofüüsikalise aktiivsuse ennustus
Geomagnetic field activity is expected to be at quiet to unsettled levels during most of the period. However, brief active conditions will be possible early in the period due to coronal hole effects.
III. Sündmuste tõenäosus 20 Jankuni 22 Jan
Klass M40%40%40%
Klass X05%05%05%
Prooton01%01%01%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       19 Jan 214
  Prognoositud   20 Jan-22 Jan  220/225/230
  90 päeva keskmine        19 Jan 223
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 18 Jan  005/005
  Hinnanguline     Afr/Ap 19 Jan  012/012
  Prognoositud    Afr/Ap 20 Jan-22 Jan  012/010-010/010-008/008
VI. Geomagnetilised aktiivsuse tõenäosused 20 Jan kuni 22 Jan
A. Keskmistel laiuskraadidel
Aktiivne35%30%20%
Väike torm10%05%01%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne45%35%25%
Väike torm15%10%05%
Suur-tõsine torm05%05%01%

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