Vaata reede, 5 august 2011 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 2011 Aug 05 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 217 Välja antud 2200Z kuni 05 Aug 2011

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 04-2100Z kuni 05-2100Z

Solar activity was low. Only low level C-flares were observed. Region 1261 (N14W64) was the major producer for C-flare activity. Region 1261 has decayed greatly in area and is now classified a Dsi spot class with a Beta-Gamma magnetic configuration. Region 1263 (N16W31) has remained largely unchanged and maintains a Beta-Gamma-Delta magnetic configuration. New Region 1267 (S17E26) was numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low with a chance for M-flares from Regions 1261 or 1263.
IIA. Summaarne geofüüsikaline aktiivsus 04-2100Z kuni 05-2100Z
The geomagnetic field began the period at unsettled levels from 04/2100-05/0300Z. Quiet levels prevailed until after 1800Z. From 1800-2100Z, minor to severe storm levels dominated. Solar wind data from ACE showed a shock-like feature passing ACE at 04/2105Z which was followed by a 20 nT sudden impulse at 04/2155Z. The solar phi angle showed rotation from negative to positive between 0300-1400Z. An additional shock passage was seen at ACE at 1722Z followed by a noticeable increase in solar wind density, velocity and magnetic field. An additional enhancement in the solar wind parameters was observed at 1834Z which include Bz fluctuation to -20 nT. Although the interpretation is not yet certain, timing analysis and model simulation suggest that the 1722Z & 1834Z enhancements are the first two of the three expected CME passages. GOES 15 observed magnetopause crossings between 1900Z-1915Z and 2000Z-2030Z. GOES 13 also observed magnetopause crossings between 2000Z-2030Z. The greater than 10 MeV proton event that began at 04/0635Z reached a peak of 83 PFU at 05/1755Z and continues in progress.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to reach minor to major storm levels with a chance for severe storm periods on 06 August. Heightened activity is expected due to continued effects from the CMEs of 02, 03, and 04 August. Activity is expected to decrease to unsettled to active levels on 07 August. Quiet to unsettled conditions are expected on 08 August.
III. Sündmuste tõenäosus 06 Augkuni 08 Aug
Klass M40%40%35%
Klass X10%10%05%
Prooton95%50%25%
PCAFred
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       05 Aug 109
  Prognoositud   06 Aug-08 Aug  110/110/100
  90 päeva keskmine        05 Aug 096
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 04 Aug  003/004
  Hinnanguline     Afr/Ap 05 Aug  020/020
  Prognoositud    Afr/Ap 06 Aug-08 Aug  035/035-015/018-008/010
VI. Geomagnetilised aktiivsuse tõenäosused 06 Aug kuni 08 Aug
A. Keskmistel laiuskraadidel
Aktiivne20%25%10%
Väike torm40%15%05%
Suur-tõsine torm35%05%00%
B. Kõrgetel laiuskraadidel
Aktiivne20%25%15%
Väike torm35%20%05%
Suur-tõsine torm40%15%00%

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