Vaata kolmapäev, 29 detsember 2004 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 2004 Dec 29 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 364 Välja antud 2200Z kuni 29 Dec 2004

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 28-2100Z kuni 29-2100Z

Solar activity increased to moderate levels today. Region 715 (N04E61) produced the largest flare of the period, an M2 x-ray flare that occurred at 29/1627Z. An associated Tenflare (510 sfu) and a spectral Type II radio sweep with an estimated shock velocity of 411 km/s. This flare also produced a CME that does appear to be Earth directed. Several lesser C-class flares were also reported from this region during the period. The large asymmetrical sunspot contains both polarities and appears to be magnetically complex. Region 713 (S09W91) produced an M1 x-ray flare that occurred at 29/1920Z. Multiple lesser C-class flares originated from this region and the sunspot cluster was in a growth phase as the spot group transited the solar west limb. No new regions were numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at low to moderate levels. Region 715 is capable of producing isolated M-class flare activity.
IIA. Summaarne geofüüsikaline aktiivsus 28-2100Z kuni 29-2100Z
The geomagnetic field was at quiet to active levels. The elevated conditions were most likely the result of the geoeffective transequatorial high speed coronal hole stream that had a mean radial speed today of approximately 430km/s. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at predominantly quiet to unsettled levels throughout the period. Isolated active conditions early on the first day (30 Dec) of the period are possible as the coronal hole rotates out of geoeffective position.
III. Sündmuste tõenäosus 30 Deckuni 01 Jan
Klass M60%50%50%
Klass X10%10%10%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       29 Dec 099
  Prognoositud   30 Dec-01 Jan  100/100/105
  90 päeva keskmine        29 Dec 105
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 28 Dec  012/016
  Hinnanguline     Afr/Ap 29 Dec  018/022
  Prognoositud    Afr/Ap 30 Dec-01 Jan  008/008-008/008-008/008
VI. Geomagnetilised aktiivsuse tõenäosused 30 Dec kuni 01 Jan
A. Keskmistel laiuskraadidel
Aktiivne20%20%20%
Väike torm01%01%01%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne20%20%20%
Väike torm05%05%05%
Suur-tõsine torm01%01%01%

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