Vaata neljapäev, 8 september 2005 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 2005 Sep 08 2204 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 251 Välja antud 2200Z kuni 08 Sep 2005IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 07-2100Z kuni 08-2100Z Solar activity remains at high levels. An X5/2b flare
was in progress from Region 808 (S09E67) at the time of this
writing. Moderate centimetric radio bursts are also in progress,
including a 990 sfu Tenflare. Very active Region 808 is rotating
into view as a large and complex sunspot cluster. Limb proximity is
still hindering the analysis, but this compact spot group will
likely exceed 1000 millionths of white light area. Numerous C-class
flares and two M2 flares preceded the X5 event. New Region 809
(N10E60) was numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to remain
at high levels. Region 808 is a large and complex sunspot group
capable of producing M and X-class flares.
IIA. Summaarne geofüüsikaline aktiivsus 07-2100Z kuni 08-2100Z
The geomagnetic field was quiet to unsettled. A sudden disturbance of
41 nT (magnetic crochet) was observed in the geomagnetic field
following today's X5 flare. A greater than 10 and greater than 100
MeV proton event occurred following yesterday's X17 flare on the
southeast limb. The greater than 10 MeV proton event began at
08/0215Z and remains in progress. The peak flux so far was 87 pfu at
08/1950Z. The greater than 100 MeV proton event began at 08/0405Z
and also remains in progress. The peak flux was 7 pfu at 08/1925Z.
A greater than 100 MeV proton event from a source on the east
limb is extremely rare. The greater than 2 MeV electron flux at
geosynchronous orbit was at high levels again today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to range from quiet to minor storm levels. The CME
associated with yesterday's X17 flare was very large and very fast.
Although the magnetic cloud associated with this CME is not expected
to impact Earth, a shock passage is expected, which will likely
produce active to minor storm periods on 09 Sep. Isolated active
periods are expected on 10 and 11 Sep. The greater than 10 MeV
proton event currently in progress is expected to continue through
10 Sep. A further enhancement in the greater than 10 MeV protons
will likely follow the anticipated shock passage on 09 Sep. Today's
X5 flare may enhance the existing proton event. The greater than 100
MeV proton event will persist through 09 Sep.
III. Sündmuste tõenäosus 09 Sepkuni 11 Sep
| Klass M | 80% | 80% | 80% |
| Klass X | 50% | 50% | 50% |
| Prooton | 99% | 90% | 75% |
| PCAF | in progress | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 08 Sep 094 Prognoositud 09 Sep-11 Sep 100/110/110 90 päeva keskmine 08 Sep 091
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 07 Sep 018/015 Hinnanguline Afr/Ap 08 Sep 008/012 Prognoositud Afr/Ap 09 Sep-11 Sep 020/025-015/020-008/010
VI. Geomagnetilised aktiivsuse tõenäosused 09 Sep kuni 11 Sep
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 40% | 30% | 25% |
| Väike torm | 20% | 15% | 10% |
| Suur-tõsine torm | 10% | 05% | 01% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 50% | 40% | 30% |
| Väike torm | 30% | 20% | 15% |
| Suur-tõsine torm | 15% | 10% | 05% |
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