Vaata reede, 16 november 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 Nov 16 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 321 Välja antud 2200Z kuni 16 Nov 2012

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 15-2100Z kuni 16-2100Z

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C8 flare observed at 16/1539Z from the northeast limb. This event was accompanied by a Type II radio sweep (511 km/s). A long duration C1 flare from Region 1613 (S23W05) occurred at 16/0751Z with an associated 24 degree filament eruption centered near S39E22 at 16/0720Z. Another filament eruption was observed from the East limb seen in SDO/AIA 304 imagery beginning at 16/0648 UTC. Analysis of SOHO/LASCO C2 suggested these eruptions would not be geoeffective. Yesterdays general trend of decreasing size and complexity continued among all active regions, leaving Region 1610 (S22W63) as the only beta-gamma type group on the visible disk. However, flux emergence was observed in other portions of the disk. New Region 1617 (S18W18) was numbered today, and emerging flux was noted near N12E35 on SDO/HMI magnetogram loops and later reported by Holloman Solar Observatory There are currently 8 numbered sunspot regions on the disk.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at low levels with a chance for an isolated moderate event on days one, two, and three (17 Nov, 18 Nov, 19 Nov).
IIA. Summaarne geofüüsikaline aktiivsus 15-2100Z kuni 16-2100Z
The geomagnetic field has been at quiet levels for the past 24 hours. Solar wind speed at the ACE spacecraft reached a peak speed of 453 km/s at 16/1112Z, but generally remained in the low to mid 400 km/s range under the waning influence of a weak negative coronal hole high speed stream. Bz was generally -4nT or greater through the period. No significant discontinuities were observed in the measured variables.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at quiet to unsettled levels for the next three days (17 Nov, 18 Nov, 19 Nov). The field is expected to be occasionally unsettled over the next three days as another coronal hole high speed stream becomes geoeffective.
III. Sündmuste tõenäosus 17 Novkuni 19 Nov
Klass M25%25%25%
Klass X05%05%05%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       16 Nov 138
  Prognoositud   17 Nov-19 Nov 141/145/145
  90 päeva keskmine        16 Nov 120

V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 15 Nov  003/003
  Hinnanguline     Afr/Ap 16 Nov  005/005
  Prognoositud    Afr/Ap 17 Nov-19 Nov  008/008-007/008-006/005

VI. Geomagnetilised aktiivsuse tõenäosused 17 Nov kuni 19 Nov
A. Keskmistel laiuskraadidel
Aktiivne20%10%05%
Väike torm10%05%01%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne15%15%15%
Väike torm30%20%10%
Suur-tõsine torm35%20%05%

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