Vaata laupäev, 13 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 13 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 287 Välja antud 2200Z kuni 13 Oct 2012

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 12-2100Z kuni 13-2100Z

Solar activity was very low. Region 1589 (N13E22) is the most magnetically complex spot group on the visible disk with a Beta-Gamma-Delta magnetic configuration. No Earth-directed CMEs were observed during the reporting period.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low with a chance for M-class flares and a slight chance for X-class flares during the forecast period (14-16 October).
IIA. Summaarne geofüüsikaline aktiivsus 12-2100Z kuni 13-2100Z
The geomagnetic field ranged from quiet to minor storm levels with major to severe storm periods observed at high latitudes. The period began with quiet to unsettled conditions through 13/0300Z. A sustained period of southward Bz to -11 nT for approximately 13 hours resulted in active to minor storm conditions with major to severe storm periods at high latitudes. At about 13/0650Z, the phi angle changed from a negative (toward) orientation to a positive (away) orientation, indicating a solar sector boundary crossing. This was followed by increases in density, temperature, and solar wind speed indicative of a co-rotating interaction region in advance of a coronal hole high speed stream (CH HSS). By 13/1618Z, solar wind speed increased from approximately 530 km/s to 590 km/s while the total magnetic field (Bt) decreased to 5 nT as the CH HSS became geoeffective. 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 continue at unsettled to active levels with a chance for isolated minor storm periods on day 1 (14 October). Mostly unsettled conditions are expected on day 2 (15 October) due to persistence. By day 3 (16 October), quiet to unsettled conditions are expected as coronal hole effects wane. On days 2-3, there is a slight chance for a greater than 10 MeV proton event at geosynchronous orbit as Region 1589 rotates into a more geoeffective position.
III. Sündmuste tõenäosus 14 Octkuni 16 Oct
Klass M35%35%35%
Klass X10%10%10%
Prooton05%10%10%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       13 Oct 125
  Prognoositud   14 Oct-16 Oct  125/130/130
  90 päeva keskmine        13 Oct 117
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 12 Oct  012/014
  Hinnanguline     Afr/Ap 13 Oct  025/036
  Prognoositud    Afr/Ap 14 Oct-16 Oct  016/018-011/012-007/010
VI. Geomagnetilised aktiivsuse tõenäosused 14 Oct kuni 16 Oct
A. Keskmistel laiuskraadidel
Aktiivne30%30%15%
Väike torm20%10%05%
Suur-tõsine torm05%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne10%15%15%
Väike torm25%30%20%
Suur-tõsine torm55%40%20%

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