Vaata neljapäev, 16 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 16 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 228 Välja antud 2200Z kuni 16 Aug 2001

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

Solar activity from numbered regions on the visible disk was low. Impulsive B- and C-class flares were observed throughout the period, the largest being an optically uncorrelated C3 flare at 16/0957 UTC. However, the most impressive activity of the day was a remarkable backside CME, observed on SOHO/LASCO starting at about 15/2355 UTC. This event resulted in the proton enhancements discussed in section IIA below. The observed CME together with backside imagery inferred from the SOHO/MDI instrument suggest old Region 9557 (S20, L=283) as the likely source, presently located near the far backside central meridian. On the visible disk, three new regions were numbered today: 9583 (S23E13), 9584 (S11E60), and 9585 (N15E74). All appear to be small, simply structured beta-class groups with low flare activity potential.
IB. Päikese aktiivsuse ennustus
Solar activity on the visible disk is expected to persist at mainly low levels for the next three days.
IIA. Summaarne geofüüsikaline aktiivsus 15-2100Z kuni 16-2100Z
Geomagnetic field activity has been quiet to unsettled throughout the period. A major proton event for >= 100MeV protons above 1pfu began at 16/0105 UTC, followed by >= 10Mev protons above 10pfu at 16/0135 UTC. Maximum flux for 100Mev protons was 29pfu at 16/0305 UTC, and for 10MeV protons was 493pfu at 16/0355 UTC. Both events remain in progress, and represent a record response for a presumed CME source so far behind the western limb as described in section 1A above. Greater than 2MeV electrons were observed at moderate enhancement levels again today, although the electron sensor on GOES-8 was saturated by the proton event for much of the period.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at active to minor storm levels within 24 hours, in response to anticipated shock passage from CME activity reported on August 14th. Isolated major storm periods may also be possible at higher latitudes, as well as an enhancement of 10MeV proton levels for the event in progress. Geomagnetic storm activity is expected to wane during day two, along with the 100MeV proton event. The 10MeV proton event is expected to persist at levels above 10pfu into day three. Greater than 2MeV electrons are also expected to persist at moderate enhancement levels.
III. Sündmuste tõenäosus 17 Augkuni 19 Aug
Klass M25%25%25%
Klass X01%01%01%
Prooton99%95%90%
PCAFred
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       16 Aug 143
  Prognoositud   17 Aug-19 Aug  140/140/145
  90 päeva keskmine        16 Aug 151
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 15 Aug  004/009
  Hinnanguline     Afr/Ap 16 Aug  007/008
  Prognoositud    Afr/Ap 17 Aug-19 Aug  025/020-017/015-012/018
VI. Geomagnetilised aktiivsuse tõenäosused 17 Aug kuni 19 Aug
A. Keskmistel laiuskraadidel
Aktiivne35%30%25%
Väike torm20%15%10%
Suur-tõsine torm10%05%05%
B. Kõrgetel laiuskraadidel
Aktiivne40%30%30%
Väike torm20%15%15%
Suur-tõsine torm05%05%05%

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