Vaata teisipäev, 23 juuli 2002 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 2002 Jul 23 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 204 Välja antud 2200Z kuni 23 Jul 2002IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 22-2100Z kuni 23-2100Z Solar activity was high. Region 39 (S15E59) produced
an X4/2b event at 23/0035 UTC with associated Type II and Type IV
radio sweeps and an 1800 sfu Tenflare. A full-halo CME was visible
in the SOHO/LASCO imagery with this event. This region now exceeds
900 millionths of white light area with a magnetic delta
configuration. Another region of interest is Region 36 (S07W28).
It also exceeds 900 millionths of white light with a magnetic
beta-gamma configuration. Two new regions were numbered today as
Regions 43 (N12E56) and 44 (S19E57).
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be
moderate to high. Regions 36 and 39 both have potential to produce
isolated major events.
IIA. Summaarne geofüüsikaline aktiivsus 22-2100Z kuni 23-2100Z
The geomagnetic field has been quiet to unsettled. Isolated active
to minor storm conditions were observed at high latitudes. The
greater than 10 MeV proton event which began at 22/0655 UTC
continues with the tentative maximum of 28 pfu at 23/1025 UTC. The
energetic electron fluxes at geosynchronous orbit were at high
levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be quiet to active on 24 July. Minor storm conditions
are expected on 25 July with active to minor conditions on 26 July.
These conditions are anticipated due to the X-class event observed
today. The greater than 10 MeV proton event is expected to continue
for most of the period. The energetic electron fluxes at
geosynchronous orbit are expected to remain at high levels for the
next several days.
III. Sündmuste tõenäosus 24 Julkuni 26 Jul
| Klass M | 75% | 75% | 75% |
| Klass X | 25% | 25% | 25% |
| Prooton | 99% | 99% | 99% |
| PCAF | yellow | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 23 Jul 198 Prognoositud 24 Jul-26 Jul 195/195/200 90 päeva keskmine 23 Jul 162
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 22 Jul 012/020 Hinnanguline Afr/Ap 23 Jul 015/015 Prognoositud Afr/Ap 24 Jul-26 Jul 015/015-030/040-020/030
VI. Geomagnetilised aktiivsuse tõenäosused 24 Jul kuni 26 Jul
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 25% | 40% | 30% |
| Väike torm | 05% | 30% | 15% |
| Suur-tõsine torm | 01% | 10% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 30% | 50% | 40% |
| Väike torm | 10% | 40% | 20% |
| Suur-tõsine torm | 05% | 10% | 10% |
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