Vaata reede, 27 september 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 Sep 27 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 270 Välja antud 2200Z kuni 27 Sep 2002

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 26-2100Z kuni 27-2100Z

Solar activity was moderate during the past 24 hours. Region 134 (N11E38) showed a marked increase in flare productivity during the past 24 hours, including two M-class events. The first was an M1/Sf at 1312 UTC and the second was an M1/Sf at 1942 UTC. Coronagraph data show a relatively narrow CME off the northeast limb in association with the first M-class event. Insufficient data were available at forecast issue time to make any CME association with the second M-class event. Analysis of the Region 134 shows the development of a small delta configuration along an east-west inversion line, and observations indicate the build up of magnetic shear in this part of the region. The only other flare-producing region on the disk was Region 132 (N19W65), which managed to produce a couple C-class subflares, but appeared to be in a state of decline. New Region 135 (S26E06) emerged on the disk today as a simple D-type sunspot group.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low to moderate. There is a fair chance for additional M-class events from Region 134, and there is a slight chance that Region 132 may produce an isolated M-class event as well.
IIA. Summaarne geofüüsikaline aktiivsus 26-2100Z kuni 27-2100Z
The geomagnetic field has been quiet to unsettled during the past 24 hours.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be quiet to unsettled for the next 24-36 hours. An increase to unsettled to slightly active is expected late on the second day and should last through the third day in response to a favorably positioned coronal hole.
III. Sündmuste tõenäosus 28 Sepkuni 30 Sep
Klass M50%50%50%
Klass X05%05%05%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       27 Sep 152
  Prognoositud   28 Sep-30 Sep  150/145/140
  90 päeva keskmine        27 Sep 179
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 26 Sep  003/008
  Hinnanguline     Afr/Ap 27 Sep  005/008
  Prognoositud    Afr/Ap 28 Sep-30 Sep  005/008-010/012-015/015
VI. Geomagnetilised aktiivsuse tõenäosused 28 Sep kuni 30 Sep
A. Keskmistel laiuskraadidel
Aktiivne15%35%35%
Väike torm10%15%20%
Suur-tõsine torm05%05%10%
B. Kõrgetel laiuskraadidel
Aktiivne20%30%40%
Väike torm15%20%25%
Suur-tõsine torm05%15%20%

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