Vaata esmaspäev, 29 märts 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 Mar 29 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 089 Välja antud 2200Z kuni 29 Mar 2004

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 28-2100Z kuni 29-2100Z

Solar activity was low. Region 582 (N14E18) produced several C-class flares today. The largest was a C5/Sf at 1551 UTC. The region dominates the solar disk in size and complexity and became more active during the past 24 hours. The region appears to be growing slowly. The only other region producing flares was 587 (S12E63) which managed to produce two B-class events. All the other regions on the disk were quiet and stable. A CME was observed by LASCO off the southwest limb around 0040 UTC, but the lack of corresponding disk signatures suggests that the source was on the back side.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be mostly low. There is a chance, however, for an isolated M-class flare from Region 582 during the next three days (30 March - 1 April).
IIA. Summaarne geofüüsikaline aktiivsus 28-2100Z kuni 29-2100Z
The geomagnetic field was mostly quiet to unsettled, although there was one active period from 0300-0600 UTC. Solar wind data show a declining high speed stream with velocities slowly decreasing over the past 24 hours. The interplanetary magnetic field shows weak fluctuations in Bz, ranging from -3 nT to +3 nT. The greater than 2 MeV electron flux was high during the past 24 hours.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be unsettled with a slight chance for an active period during the next 24 hours (30 March). Conditions should decline to quiet to unsettled for the second and third days (31 March - 1 April) as the solar wind returns to nominal conditions.
III. Sündmuste tõenäosus 30 Markuni 01 Apr
Klass M35%35%35%
Klass X05%05%05%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       29 Mar 129
  Prognoositud   30 Mar-01 Apr  130/130/135
  90 päeva keskmine        29 Mar 111
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 28 Mar  012/017
  Hinnanguline     Afr/Ap 29 Mar  012/013
  Prognoositud    Afr/Ap 30 Mar-01 Apr  012/012-010/008-005/008
VI. Geomagnetilised aktiivsuse tõenäosused 30 Mar kuni 01 Apr
A. Keskmistel laiuskraadidel
Aktiivne30%25%20%
Väike torm20%15%10%
Suur-tõsine torm05%05%05%
B. Kõrgetel laiuskraadidel
Aktiivne30%25%20%
Väike torm25%20%15%
Suur-tõsine torm10%05%05%

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