Vaata pühapäev, 15 aprill 2001 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 2001 Apr 15 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 105 Välja antud 2200Z kuni 15 Apr 2001

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 14-2100Z kuni 15-2100Z

Solar activity was high. Region 9415 (S12W87) produced an X14/2b flare at 15/1350 UTC. This event had an associated Type II, with a speed of 1000 km/s, and Type IV radio sweeps. It was also accompanied by a tenflare of 48000 sfu. A 12 degree filament located at S23W02 disappeared between 14/2054 UTC and 15/1135 UTC.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low to moderate. Region 9415 is still capable of producing a major flare before it rotates over the western limb.
IIA. Summaarne geofüüsikaline aktiivsus 14-2100Z kuni 15-2100Z
The geomagnetic field was unsettled to active. The X-class event described in Part IA produced proton events at greater than 10 and 100 MeV flux at geosynchronous orbit which are still in progress. The greater than 100 MeV crossed event threshold at 15/1405 UTC, and so far have reached a peak flux of 146 pfu at 15/1525 UTC. The greater than 10 MeV crossed event threshold at 15/1410 UTC and has reached a peak flux of 951 pfu at 15/1920 UTC. A ground level event was measured on the Thule riometer at 15/1505 UTC, and a polar cap absorption (PCA) event began at 15/1950 UTC.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be quiet to active for April 16 and 17. Active to minor storm conditions are expected on April 18 as a result of the X14 mentioned in Part IA above. Effects from a high speed coronal stream may also be expected on April 18. The greater than 10 MeV proton event is expected to continue for most of the period, and the greater than 100 MeV proton event is expected to go below threshold by sometime on April 16.
III. Sündmuste tõenäosus 16 Aprkuni 18 Apr
Klass M80%70%60%
Klass X25%10%10%
Prooton90%10%10%
PCAFin progress
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       15 Apr 134
  Prognoositud   16 Apr-18 Apr  145/150/160
  90 päeva keskmine        15 Apr 166
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 14 Apr  013/015
  Hinnanguline     Afr/Ap 15 Apr  015/015
  Prognoositud    Afr/Ap 16 Apr-18 Apr  015/015-015/020-020/035
VI. Geomagnetilised aktiivsuse tõenäosused 16 Apr kuni 18 Apr
A. Keskmistel laiuskraadidel
Aktiivne25%25%50%
Väike torm05%05%10%
Suur-tõsine torm01%01%05%
B. Kõrgetel laiuskraadidel
Aktiivne30%35%60%
Väike torm10%10%15%
Suur-tõsine torm05%05%10%

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