Vaata pühapäev, 11 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 11 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 102 Välja antud 2200Z kuni 11 Apr 2004

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 10-2100Z kuni 11-2100Z

Solar activity was low. Region 588 (S15W55) produced a C9/1F flare and an associated filament eruption at 11/0419Z. Moderate centimetric radio bursts accompanied this flare including a 920 sfu tenflare. A greater than 10 MeV proton event that began at 11/1135Z is also believed to be associated with this eruption. A CME was observed on LASCO imagery and a preliminary analysis indicates that while most of the ejecta is directed south and west, there is an Earthward directed component. Region 588 is still the only sunspot group on the visible disk and maintains a reverse polarity beta magnetic configuration.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low to very low. Region 588 may produce isolated C-class flares.
IIA. Summaarne geofüüsikaline aktiivsus 10-2100Z kuni 11-2100Z
The geomagnetic field was quiet to unsettled. Solar wind speed began the period at elevated levels (over 500 km/s) following yesterday's shock arrival at 10/1925Z. However, IMF Bz stayed predominantly northward and as a result, the geomagnetic disturbance was weak. Solar wind speed dropped to around 430 km/s by the end of the period. A greater than 10 MeV proton event began at 11/1135Z. The peak so far was 35 pfu at 11/1845Z.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to range from quiet to minor storm levels. A CME associated with the C2 flare at 09/2040Z is expected to produce occasional active periods on 12 April. Mostly quiet to unsettled conditions are expected on 13 April. Active conditions with high latitude minor storm periods are expected on 14 April in response to today's C9 flare and CME. The greater than 10 MeV proton event in progress now is expected to end on 12 April.
III. Sündmuste tõenäosus 12 Aprkuni 14 Apr
Klass M15%15%15%
Klass X01%01%01%
Prooton75%10%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       11 Apr 090
  Prognoositud   12 Apr-14 Apr  095/100/105
  90 päeva keskmine        11 Apr 109
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 10 Apr  010/010
  Hinnanguline     Afr/Ap 11 Apr  010/012
  Prognoositud    Afr/Ap 12 Apr-14 Apr  012/015-010/015-018/025
VI. Geomagnetilised aktiivsuse tõenäosused 12 Apr kuni 14 Apr
A. Keskmistel laiuskraadidel
Aktiivne30%25%35%
Väike torm15%10%20%
Suur-tõsine torm05%05%10%
B. Kõrgetel laiuskraadidel
Aktiivne35%30%40%
Väike torm20%15%25%
Suur-tõsine torm10%05%15%

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