Vaata esmaspäev, 16 juuni 2003 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 2003 Jun 16 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 167 Välja antud 2200Z kuni 16 Jun 2003IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 15-2100Z kuni 16-2100Z Solar activity was very high. New Region 386 (S07E71)
produced an X1/Sf flare at 15/2356 UTC with an associated Type II
(841 km/s) and Type IV radio sweep. SOHO/LACSO imagery indicates a
full halo CME, however the majority of the ejecta was off to the
east. Region 386 currently indicates a beta magnetic configuration
but its proximity to the east limb prevents a detailed analysis of
the magnetic complexity. Region 380 (S16W51) has slowed its rate of
decay and has developed a beta-gamma magnetic configuration. New
Region 386 was numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at
moderate to high levels. Region 386 is expected to produce M-class
and possibly X-class activity.
IIA. Summaarne geofüüsikaline aktiivsus 15-2100Z kuni 16-2100Z
The geomagnetic field was at unsettled to minor storm levels. The
source of the minor storm conditions may be associated with the
Boulder magnetometer scaling problem (see comment in VII). Solar
wind speed was in gradual decay from a peak near 600 km/s early in
the day to a minimum of 450 km/s by 1600UTC. Wind speed then
increased to 550 km/s by the end of the day.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be quiet to active with a chance of isolated minor storm
levels. Late on day one or early on day two, weak CME shock effects
are possible from the X1 event mentioned in IA. A coronal hole high
speed flow is expected late on day two and day three with isolated
minor storm levels possible.
III. Sündmuste tõenäosus 17 Junkuni 19 Jun
| Klass M | 50% | 50% | 50% |
| Klass X | 20% | 20% | 20% |
| Prooton | 30% | 20% | 20% |
| PCAF | green | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 16 Jun 123 Prognoositud 17 Jun-19 Jun 125/125/120 90 päeva keskmine 16 Jun 124
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 15 Jun 013/020 Hinnanguline Afr/Ap 16 Jun 014/023 Prognoositud Afr/Ap 17 Jun-19 Jun 012/015-020/030-020/030
VI. Geomagnetilised aktiivsuse tõenäosused 17 Jun kuni 19 Jun
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 25% | 30% | 35% |
| Väike torm | 10% | 15% | 15% |
| Suur-tõsine torm | 05% | 05% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 30% | 40% | 40% |
| Väike torm | 15% | 20% | 25% |
| Suur-tõsine torm | 05% | 10% | 15% |
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