Vaata neljapäev, 12 juuli 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 Jul 12 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 194 Välja antud 2200Z kuni 12 Jul 2012

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 11-2100Z kuni 12-2100Z

Solar activity was high. At 12/1649Z, a long-duration X1/2b flare was observed from Region 1520 (S16W09). The event was visible in GONG H-alpha imagery as a bright ribbon flare that erupted along the region?s long E/W oriented inversion line. Associated with this event were Type II (1268 km/s) and Type IV radio emissions along with an 800 sfu Tenflare. Limited satellite imagery indicated a CME was associated with this event. STEREO Behind COR2 imagery observed a CME lifting off the west limb, first visible at 12/1710Z. Further analysis of this CME is ongoing. During the past 24 hours, Region 1520 grew in both area and spot count and maintained a complex beta-gamma-delta magnetic configuration. Region 1521 (S21W21) also grew in area and spot count and remained a beta-gamma magnetic classification. New Regions 1522 (N13W21) and 1523 (S27E31) emerged on the disk as simple bi-polar spot groups.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be moderate with a chance for X-class events for the next three days (13 - 15 July).
IIA. Summaarne geofüüsikaline aktiivsus 11-2100Z kuni 12-2100Z
The geomagnetic field was at quiet to active levels with isolated high latitude major storm intervals from 11/0600 - 1200Z. ACE solar data indicated wind velocities decreased steadily through the period from 500 km/s to near 400 km/s while the Bz component of the interplanetary magnetic field did not vary much beyond +/- 5 nT. The greater than 10 MeV proton flux at geosynchronous orbit exceeded the 10 pfu event threshold at 12/1835Z. At the time of this report, flux levels were at 35 pfu and rising. The greater than 100 MeV flux at geosynchronous orbit was enhanced, but below event threshold levels of 1 pfu. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at mostly quiet to unsettled levels for day one (13 July). Unsettled to active levels, with isolated minor storm intervals, are expected on days two and three (14 - 15 July) as effects from the 12 July CME are expected to become geoeffective.
III. Sündmuste tõenäosus 13 Julkuni 15 Jul
Klass M80%80%80%
Klass X35%35%35%
Prooton99%99%50%
PCAFred
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       12 Jul 165
  Prognoositud   13 Jul-15 Jul  165/165/165
  90 päeva keskmine        12 Jul 127
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 11 Jul  010/012
  Hinnanguline     Afr/Ap 12 Jul  009/011
  Prognoositud    Afr/Ap 13 Jul-15 Jul  006/008-015/018-013/015
VI. Geomagnetilised aktiivsuse tõenäosused 13 Jul kuni 15 Jul
A. Keskmistel laiuskraadidel
Aktiivne20%40%35%
Väike torm05%15%10%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne20%10%15%
Väike torm25%30%30%
Suur-tõsine torm25%55%45%

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