Vaata laupäev, 14 oktoober 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 Oct 14 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 288 Välja antud 2200Z kuni 14 Oct 2000

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 13-2100Z kuni 14-2100Z

Solar activity has been moderate. Region 9182 (N04W90) produced an M1/Sf flare at 14/0840 UTC, as well as several C-class subfaint flares. Region 9194 (S12E36) exhibited some increased activity today, also producing several C-class subfaint flares. Single flares of similar magnitude were noted from a few other regions, including newly numbered Region 9198 (S30E65).
IB. Päikese aktiivsuse ennustus
Solar activity is expected to become predominantly low, with the departure of Region 9182 behind the western limb. A chance of isolated moderate-level activity remains for regions 9194, 9193 (N05W46), and for new regions expected on the eastern limb.
IIA. Summaarne geofüüsikaline aktiivsus 13-2100Z kuni 14-2100Z
The geomagnetic field varied from unsettled to major storm levels, due to a prolonged period of negative Bz accompanied by moderate solar wind speed. Greatest activity occurred during 14/0900-1800 UTC, which saw two periods of storming at minor levels in middle latitudes, and at major levels in higher latitudes. Possible sources of this activity include extended effects of the 09 October CME passage, which commenced yesterday, or trailing effects from a weaker LDE C-flare that occurred about 30 hours after the CME.
IIB. Geofüüsikalise aktiivsuse ennustus
Geomagnetic activity is expected to ease to unsettled levels, with isolated active periods. The current geomagnetic disturbance is expected to end during day one, and an onset of high speed stream effects from a coronal hole is expected to emerge thereafter, persisting through day two and tapering off during day three. Isolated minor storming at higher latitudes is possible during this period.
III. Sündmuste tõenäosus 15 Octkuni 17 Oct
Klass M30%30%30%
Klass X05%05%05%
Prooton01%01%01%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       14 Oct 163
  Prognoositud   15 Oct-17 Oct  175/185/195
  90 päeva keskmine        14 Oct 177
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 13 Oct  022/027
  Hinnanguline     Afr/Ap 14 Oct  028/040
  Prognoositud    Afr/Ap 15 Oct-17 Oct  018/020-015/015-015/015
VI. Geomagnetilised aktiivsuse tõenäosused 15 Oct kuni 17 Oct
A. Keskmistel laiuskraadidel
Aktiivne30%30%25%
Väike torm10%10%10%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne35%35%30%
Väike torm15%15%10%
Suur-tõsine torm05%05%01%

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