Vaata esmaspäev, 11 oktoober 2010 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 2010 Oct 11 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 284 Välja antud 2200Z kuni 11 Oct 2010

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 10-2100Z kuni 11-2100Z

Solar activity was very low. Region 1112 (S19E40) showed little change during the period. SDO/AIA 193 imagery observed a filament eruption at approximately 10/2121Z. The filament was 17 degrees long and centered near S08E48, just north of Region 1112. A slow-moving, CME was detected at 11/0012Z by SOHO LASCO c2 imagery and did not appear to be Earth-directed.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to remain very low with a slight chance for C-class activity.
IIA. Summaarne geofüüsikaline aktiivsus 10-2100Z kuni 11-2100Z
The geomagnetic field ranged from quiet to minor storm levels. Activity levels were quiet through 11/0600Z. By 11/0900Z, geomagnetic activity increased at all latitudes to predominately unsettled to active levels with an isolated minor storm period observed between 11/1200 - 1500Z. At approximately 11/0300Z, measurements at the ACE spacecraft observed flucuations in the B component of the interplanetary magnetic field (IMF) along with a sharp increase in density and a slight increase in wind velocity. The IMF Bz reached a maximum of -13 nT at 11/0915Z, and remained southward through 11/1805Z. The IMF Bt hit a maximum of 14 nT at 11/0936Z while density reached a peak of 47 p/cc at 11/0509Z. Wind velocities increased slightly from a low of 325 km/s at the beginning of the summary period and peaked near 375 km/s at 11/1826Z. The increase in activity is most likely a result of a glancing blow from the 06 October full-halo CME.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be quiet to unsettled, with isolated active periods on day one (12 October) due to lingering CME effects. Mostly quiet levels are expected by days two and three (13 - 14 October).
III. Sündmuste tõenäosus 12 Octkuni 14 Oct
Klass M01%01%01%
Klass X01%01%01%
Prooton01%01%01%
PCAFGreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       11 Oct 075
  Prognoositud   12 Oct-14 Oct  076/076/076
  90 päeva keskmine        11 Oct 080
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 10 Oct  001/002
  Hinnanguline     Afr/Ap 11 Oct  012/015
  Prognoositud    Afr/Ap 12 Oct-14 Oct  008/012-005/005-005/005
VI. Geomagnetilised aktiivsuse tõenäosused 12 Oct kuni 14 Oct
A. Keskmistel laiuskraadidel
Aktiivne25%15%05%
Väike torm05%01%01%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne35%20%15%
Väike torm10%01%01%
Suur-tõsine torm01%01%01%

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