Vaata laupäev, 10 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 10 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 101 Välja antud 2200Z kuni 10 Apr 2004IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 09-2100Z kuni 10-2100Z Solar activity was very low. Region 588 (S15W38)
contains the only sunspots on the visible disk. This region
maintains a reverse polarity beta magnetic configuration, but has
been quiet since producing a C2 flare and CME at 09/2040Z. No other
significant activity or changes were observed.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low
to very low. Isolated C-class flares are possible from Region 588.
IIA. Summaarne geofüüsikaline aktiivsus 09-2100Z kuni 10-2100Z
The geomagnetic field was quiet to unsettled. Solar wind speed was in
gradual decline following yesterday's CME impact. Speed declined
from a peak near 570 km/s at 09/0505Z to near 400 km/s late in the
period. A sharp discontinuity in solar wind plasma and IMF
measurements occurred at 10/1925Z. This was likely the
interplanetary shock associated with the C7 flare and CME on 08
April. Solar wind speed following the shock ranged from 500 to 540
km/s, but the IMF BZ was mostly northward. The greater than 2 MeV
electron flux at geosynchronous orbit reached high levels again this
period.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be quiet to active. Occasional active periods are
expected on 11 April following today's CME arrival. Updated LASCO
imagery reveal another Earth-directed CME associated with
yesterday's C2 flare at 09/2040Z. A geomagnetic response is likely
on 12 April, but the disturbance should be limited to occasional
active periods. Mostly quiet to unsettled conditions are expected on
13 April.
III. Sündmuste tõenäosus 11 Aprkuni 13 Apr
| Klass M | 05% | 10% | 10% |
| Klass X | 01% | 01% | 01% |
| Prooton | 01% | 01% | 01% |
| PCAF | green | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 10 Apr 088 Prognoositud 11 Apr-13 Apr 090/095/100 90 päeva keskmine 10 Apr 109
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 09 Apr 011/016 Hinnanguline Afr/Ap 10 Apr 015/012 Prognoositud Afr/Ap 11 Apr-13 Apr 020/020-010/015-005/010
VI. Geomagnetilised aktiivsuse tõenäosused 11 Apr kuni 13 Apr
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 40% | 30% | 15% |
| Väike torm | 25% | 10% | 05% |
| Suur-tõsine torm | 15% | 01% | 01% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 45% | 35% | 25% |
| Väike torm | 35% | 15% | 10% |
| Suur-tõsine torm | 20% | 05% | 01% |
Kõik ajad UTC-s
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