Vaata teisipäev, 6 aprill 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 Apr 06 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 097 Välja antud 2200Z kuni 06 Apr 2004

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 05-2100Z kuni 06-2100Z

Solar activity has been moderate. Region 588 (S15E14) produced an M2.4/Sf flare at 06/1328 UTC. A full-halo CME was observed on LASCO imagery erupting from the sun shortly after the flare, with an estimated speed of 1050 km/s. The CME was not directed towards Earth, but may provide a glancing blow to the geomagnetic field. No significant development was observed from active regions on the visible disk, and no new regions were numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low. Region 588 may produce C- and isolated M-class flares.
IIA. Summaarne geofüüsikaline aktiivsus 05-2100Z kuni 06-2100Z
The geomagnetic field has been at quiet to minor storm conditions. After increasing early in the period, the solar wind speed has leveled off at about 575 km/s. The greater than 2 MeV electrons hovered at the high threshold for most of the day, and ended the period below the threshold.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at quiet to active conditions all three days under the continued influence of a high speed solar wind stream associated with a coronal hole in geoeffective position. Minor storm conditions are expected on day two (8 April) due to the potential effects from two recent CMEs. Although neither appeared to be directed toward Earth, the CME associated with the M1.7 flare that occurred on 5 April and the CME associated with today's M2.4 flare should both arrive early on 8 April and may come close enough to Earth's geomagnetic field to cause minor storming.
III. Sündmuste tõenäosus 07 Aprkuni 09 Apr
Klass M25%25%25%
Klass X01%01%01%
Prooton01%01%01%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       06 Apr 101
  Prognoositud   07 Apr-09 Apr  105/105/100
  90 päeva keskmine        06 Apr 110
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 05 Apr  009/014
  Hinnanguline     Afr/Ap 06 Apr  018/026
  Prognoositud    Afr/Ap 07 Apr-09 Apr  015/020-025/030-015/020
VI. Geomagnetilised aktiivsuse tõenäosused 07 Apr kuni 09 Apr
A. Keskmistel laiuskraadidel
Aktiivne30%40%30%
Väike torm20%25%20%
Suur-tõsine torm10%20%10%
B. Kõrgetel laiuskraadidel
Aktiivne30%30%30%
Väike torm35%30%35%
Suur-tõsine torm25%35%30%

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