Vaata reede, 16 august 2002 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 2002 Aug 16 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 228 Välja antud 2200Z kuni 16 Aug 2002

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 15-2100Z kuni 16-2100Z

Solar activity increased to high levels. Region 69 (S07E11) continues to grow at a gradual pace in both penumbral coverage and magnetic complexity. This region produced the largest flare during the period, a long duration M5/2n occurring at 16/1232 UTC with an associated 1600 sfu Tenflare and a Type II radio sweep with an estimated shock velocity of 1836 km/s. Moderate to strong discrete radio bursts and a strong Type IV radio sweep were also associated with this flare. SOHO/LASCO reported a full-halo CME surrounding the C2 occulting disk by 16/1254 UTC. Region 61 (now beyond the west limb) produced an M2/Sf flare at 16/0611 UTC just prior to exiting the disk. A Type II radio sweep with an estimated shock velocity of 1450 km/s was associated with this flare. Region 78 (S13W39) produced an M1/Sf at 16/2333 UTC. Newly numbered region 81 (N17E61) was assigned today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at moderate levels. Region 69 has the potential to produce further major flare activity.
IIA. Summaarne geofüüsikaline aktiivsus 15-2100Z kuni 16-2100Z
The geomagnetic field was at unsettled to minor storm levels. A slight indication of a weak shock passage at the ACE spacecraft was observed at the beginning of the period. The greater than 2 MeV electron flux at geo-synchronous orbit exceeded threshold at 16/1505 UTC, preliminary maximum flux was 1340 pfu at 16/1530 UTC.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at unsettled to active levels through most of day one of the period. Minor to major storm conditions may begin as early as day two of the period in response to the major flare and associated CME mentioned in IA. Day three should see a return to unsettled to active conditions as the potential effects from expected shock subside. The greater than 2 MeV electron flux should see a return to moderate levels by day one of the period.
III. Sündmuste tõenäosus 17 Augkuni 19 Aug
Klass M75%75%75%
Klass X15%15%15%
Prooton10%10%10%
PCAFyellow
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       16 Aug 214
  Prognoositud   17 Aug-19 Aug  215/220/225
  90 päeva keskmine        16 Aug 166
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 15 Aug  018/019
  Hinnanguline     Afr/Ap 16 Aug  020/020
  Prognoositud    Afr/Ap 17 Aug-19 Aug  020/020-050/070-018/020
VI. Geomagnetilised aktiivsuse tõenäosused 17 Aug kuni 19 Aug
A. Keskmistel laiuskraadidel
Aktiivne40%30%40%
Väike torm15%25%15%
Suur-tõsine torm10%25%10%
B. Kõrgetel laiuskraadidel
Aktiivne35%30%30%
Väike torm15%30%15%
Suur-tõsine torm15%30%15%

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