Vaata reede, 17 august 2001 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 2001 Aug 17 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 229 Välja antud 2200Z kuni 17 Aug 2001

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 16-2100Z kuni 17-2100Z

Solar activity was low. Only a few low-level C-class subflares occurred. The largest was a C1/Sf at 17/0011 UTC in Region 9581 (S25W42). Although there are several sunspot groups on the visible disk all of them are relatively small and magnetically simple. New Regions 9586 (S15W47) and 9587 (S11E56) were numbered.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low. Additional low-level C-class flares are possible.
IIA. Summaarne geofüüsikaline aktiivsus 16-2100Z kuni 17-2100Z
The geomagnetic field was quiet until the occurrence of a sudden impulse observed at ground magnetometers (36 nT at Boulder) at about 17/1103 UTC. The impulse was preceded by a shock observed at the NASA ACE spacecraft at 17/1017 UTC. The geomagnetic field has been at mostly active to minor storm levels since the impulse. A series of magnetopause crossings were observed at the NOAA GOES spacecraft in the interval from about 17/1930--2100 UTC. The greater than 100 MeV proton event which began yesterday has ended (start 16/0105 UTC, 29 pfu peak at 16/0305 UTC, and end 17/1415 UTC). The greater than 10 MeV event remains in progress (start 16/0135 UTC and 493 pfu peak at 16/0355 UTC). The current proton flux (17/2100 UTC) at greater than 10 MeV is about 20 pfu and is slowly decaying.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at mostly active to minor storm levels for the next 24 hours becoming unsettled to active after that. The greater than 10 MeV proton event is expected to end by 19 August.
III. Sündmuste tõenäosus 18 Augkuni 20 Aug
Klass M10%10%10%
Klass X01%01%01%
Prooton90%30%01%
PCAFin progress
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       17 Aug 145
  Prognoositud   18 Aug-20 Aug  150/150/155
  90 päeva keskmine        17 Aug 151
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 16 Aug  003/008
  Hinnanguline     Afr/Ap 17 Aug  025/025
  Prognoositud    Afr/Ap 18 Aug-20 Aug  020/015-015/015-010/018
VI. Geomagnetilised aktiivsuse tõenäosused 18 Aug kuni 20 Aug
A. Keskmistel laiuskraadidel
Aktiivne30%20%15%
Väike torm15%05%05%
Suur-tõsine torm05%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne40%30%20%
Väike torm20%10%05%
Suur-tõsine torm05%01%01%

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