Vaata teisipäev, 5 november 2002 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 2002 Nov 05 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 309 Välja antud 2200Z kuni 05 Nov 2002

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 04-2100Z kuni 05-2100Z

Solar activity was at low levels. Region 177 (N16W09) produced the two largest flares during the period, a C7.5/Sf event occurred at 05/1257 UTC and a slightly smaller C6.4/Sn flare maximum was recorded at 05/1610 UTC. Magnetic analysis indicates slight growth in complexity while the average white-light area is now at 390 millionths with 17 spots. Region 180 (S10E17) only managed to produce minor C-class flares today. Even so, the magnetic structure to this region has shown significant growth during the period with the dominant lead spot exhibiting a distinct delta complex. New Region 186 (N20E02) was numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at low to moderate levels. Both Regions 177 and 180 have M-class flare potential.
IIA. Summaarne geofüüsikaline aktiivsus 04-2100Z kuni 05-2100Z
The geomagnetic field was at unsettled to active levels. The Bz component of the interplanetary magnetic field remained mostly southward today. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the past 24 hours.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at unsettled to active levels into the first day of the period. The elevated solar wind speeds in response to a geoeffective high speed coronal hole stream should begin to diminish by the end of day one, returning to predominantly quiet to unsettled conditions on days two and three. The greater than 2 MeV electron flux at geosynchronous orbit should reach moderate to high levels again tomorrow, 06 November.
III. Sündmuste tõenäosus 06 Novkuni 08 Nov
Klass M50%50%50%
Klass X10%10%10%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       05 Nov 183
  Prognoositud   06 Nov-08 Nov  180/185/180
  90 päeva keskmine        05 Nov 177
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 04 Nov  011/021
  Hinnanguline     Afr/Ap 05 Nov  015/020
  Prognoositud    Afr/Ap 06 Nov-08 Nov  012/015-010/010-008/010
VI. Geomagnetilised aktiivsuse tõenäosused 06 Nov kuni 08 Nov
A. Keskmistel laiuskraadidel
Aktiivne30%25%20%
Väike torm20%15%10%
Suur-tõsine torm10%05%01%
B. Kõrgetel laiuskraadidel
Aktiivne40%30%25%
Väike torm25%15%15%
Suur-tõsine torm15%05%05%

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