Vaata pühapäev, 19 september 2004 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 2004 Sep 19 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 263 Välja antud 2200Z kuni 19 Sep 2004IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 18-2100Z kuni 19-2100Z Solar activity was moderate. Region 672 (N05W58), which
has been in a decay phase over the last 72 hours, produced two
notable events this period. The first was an extended C3.8 flare at
19/1148Z that erupted along a filament channel just north of the
spot cluster. The second was an M1.9 flare at 19/1712Z. This
impressive flare had associated Type II (604 km/s) and Type IV radio
sweeps; a 520 sfu Tenflare, and a greater than 10 MeV proton event.
LASCO imagery was unavailable. Region 672 is a C-type beta spot
group with under 100 millionths of white light area coverage. Region
673 (S13E22) showed little change this period and continues to
produce occasional B-class flare activity.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low
to very low. There is a small chance of another M-class flare from
Region 672 before it rotates around the west limb early on 22
September. Occasional C-class flares are possible from Region 673.
IIA. Summaarne geofüüsikaline aktiivsus 18-2100Z kuni 19-2100Z
The geomagnetic field was quiet. Solar wind speed was generally below
400 km/s. A greater than 10 MeV proton event followed today's M1
flare at 19/1712Z. The proton event began at 19/1925Z and was still
in progress at the time of issue. The maximum flux value so far was
35 pfu at 19/2025Z. A greater than 100 MeV proton flux enhancement
was also observed, but has not exceeded the 1 pfu event threshold.
The greater than 2 MeV electron flux at geosynchronous orbit was at
high levels.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to remain at mostly quiet to unsettled levels on 20 and 21
September. A disturbance associated with today's M1 flare and CME is
expected to occur on 22 September: Active to minor storm periods are
likely. The greater than 10 MeV proton event in progress now is
expected to end by 21 September.
III. Sündmuste tõenäosus 20 Sepkuni 22 Sep
| Klass M | 15% | 10% | 10% |
| Klass X | 01% | 01% | 01% |
| Prooton | 99% | 10% | 10% |
| PCAF | yellow | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 19 Sep 105 Prognoositud 20 Sep-22 Sep 100/095/090 90 päeva keskmine 19 Sep 112
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 18 Sep 016/016 Hinnanguline Afr/Ap 19 Sep 005/008 Prognoositud Afr/Ap 20 Sep-22 Sep 005/008-008/012-015/020
VI. Geomagnetilised aktiivsuse tõenäosused 20 Sep kuni 22 Sep
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 20% | 30% |
| Väike torm | 01% | 05% | 10% |
| Suur-tõsine torm | 01% | 01% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 20% | 25% | 40% |
| Väike torm | 05% | 10% | 20% |
| Suur-tõsine torm | 01% | 01% | 10% |
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