Vaata teisipäev, 23 oktoober 2012 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 2012 Oct 23 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 297 Välja antud 2200Z kuni 23 Oct 2012

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

Solar activity has been high. Region 1598 (S12E44) produced an X1 event with an associated Tenflare and Type-II radio sweep at 23/0317Z. There was no CME observed in association with this event. Region 1598 remains the most threatening region on the disk and appears to have a Delta magnetic configuration within its trailer spots. Region 1596 (N07E06) is also moderately sized and has some magnetic complexity, but did not produce any flares during the period. Region 1593 (N15W33) produced a long-duration C3 event at 23/0821Z with an associated CME seen on STEREO-A imagery. There is not enough data available to model the CME, but at this time it does not appear likely to be geoeffective. Newly numbered Region 1599 (S09E73) appears to have a simple alpha magnetic class. The other regions on the disk either remained stable or were decaying.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be moderate to high with occasional M-class events, and a slight chance for an isolated X-class event for the next three days (24 - 26 Oct) with Region 1598 the most likely source.
IIA. Summaarne geofüüsikaline aktiivsus 22-2100Z kuni 23-2100Z
The geomagnetic field was quiet for the past 24 hours. Solar wind speed, as measured at the ACE spacecraft, remained steady throughout the period at approximately 370 km/s. The Bz component of the interplanetary magnetic field ranged from +/- 4 nT and the Phi angle changed to a positive sector at 22/2300Z. These signatures are consistent with a solar sector boundary crossing. The greater than 2 MeV electron flux at geosynchronous orbit was at high levels throughout the period.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be quiet for the next three days (24 - 26 Oct).
III. Sündmuste tõenäosus 24 Octkuni 26 Oct
Klass M75%75%75%
Klass X20%20%20%
Prooton05%10%15%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       23 Oct 142
  Prognoositud   24 Oct-26 Oct  140/140/140
  90 päeva keskmine        23 Oct 121
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 22 Oct  002/002
  Hinnanguline     Afr/Ap 23 Oct  007/007
  Prognoositud    Afr/Ap 24 Oct-26 Oct  006/005-006/005-006/005
VI. Geomagnetilised aktiivsuse tõenäosused 24 Oct kuni 26 Oct
A. Keskmistel laiuskraadidel
Aktiivne05%05%05%
Väike torm01%01%01%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne15%15%15%
Väike torm15%15%10%
Suur-tõsine torm05%05%05%

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