Vaata esmaspäev, 24 november 2003 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 2003 Nov 24 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 328 Välja antud 2200Z kuni 24 Nov 2003

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 23-2100Z kuni 24-2100Z

Solar activity was low. Several low C-class flares were observed throughout the period. Region 501 (N03W72) is undergoing considerable decay as it approaches the west limb, but is still producing isolated C-class flares. Region 508 (S17E08) was responsible for most of the low C-class activity. No significant change was noted in this moderately complex region over the last 24 hours. It maintains a beta-gamma configuration in approximately 450 millionths of white light areal coverage. Region 507 (N09W03) is the largest and most complex region on the visible disk, but was rather quiet this period. A weak delta configuration is apparent in this spot group with over 700 millionths of areal coverage. New Regions 509 (S10E56) and 510 (S22E62) were numbered today. Region 509 produced a C2/Sf flare at 24/1854Z.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at low to moderate levels. An isolated M-class flare is possible, primarily from Regions 501, 507, and 508.
IIA. Summaarne geofüüsikaline aktiivsus 23-2100Z kuni 24-2100Z
The geomagnetic field was quiet to unsettled with isolated active periods in the higher latitudes. A well positioned coronal hole is producing solar wind speeds near 600 km/s, creating a weak disturbance in the geomagnetic field. The greater than 2 MeV electrons at geosynchronous orbit were at high levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to continue at quiet to active levels through 26 November. Isolated minor storm levels are also expected, but will be confined mostly to higher latitudes. Quiet to unsettled levels are expected on 27 November as the current disturbance subsides.
III. Sündmuste tõenäosus 25 Novkuni 27 Nov
Klass M40%40%30%
Klass X10%10%05%
Prooton05%05%05%
PCAFyellow
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       24 Nov 177
  Prognoositud   25 Nov-27 Nov  175/170/160
  90 päeva keskmine        24 Nov 132
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 23 Nov  013/021
  Hinnanguline     Afr/Ap 24 Nov  015/020
  Prognoositud    Afr/Ap 25 Nov-27 Nov  015/020-015/020-012/015
VI. Geomagnetilised aktiivsuse tõenäosused 25 Nov kuni 27 Nov
A. Keskmistel laiuskraadidel
Aktiivne40%40%30%
Väike torm20%20%15%
Suur-tõsine torm05%05%01%
B. Kõrgetel laiuskraadidel
Aktiivne50%50%40%
Väike torm25%25%20%
Suur-tõsine torm10%10%05%

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