Vaata laupäev, 20 september 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 Sep 20 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 263 Välja antud 2200Z kuni 20 Sep 2003

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 19-2100Z kuni 20-2100Z

Solar activity was low during the past 24 hours. Today's largest event was a C3.6 at 1536 UTC. There was only limited image data for this event, but it appears to have originated from newly assigned Region 464 (N05E77) which rotated into view today. Region 464 is a relatively large (360 millionths) E-type sunspot group and displayed frequent surge activity during the past 24 hours. Region 461 (N13W89), now crossing the west limb, produced the second largest event of the day, a C3 at 0512 UTC. Region 459 (S11W40) showed slow growth and occasional brightenings but was otherwise stable. LASCO images show a coronal mass ejection (CME) off the west limb, beginning at 0430 UTC. The CME does not appear to have any earthward component.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low for the next three days. Regions 464 and 459 are the most likely sources for activity. There is a slight chance for an isolated M-class flare.
IIA. Summaarne geofüüsikaline aktiivsus 19-2100Z kuni 20-2100Z
The geomagnetic field was at unsettled to minor storm levels with an isolated major storm period at some locations between 0300-0600 UTC. Geomagnetic conditions were initially unsettled from 20/2100-21/0000 UTC, but became more disturbed after 0000 UTC and remained so for the remainder of the day, with active conditions predominating. The solar wind signatures show the continued presence of a high speed coronal hole stream. In particular, the solar wind speed showed an increase around 0000 UTC up to about 700 km/s. The signature is consistent with the transition of the solar wind source from an isolated coronal hole in the western hemisphere to a southern polar extension coronal hole that crossed central meridian on 18 September. The greater than 2 MeV electron fluxes reached high levels during the past 24 hours.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be mostly active for the next 24 hours as the current coronal-hole driven disturbance continues. A slight decline to predominantly unsettled to active is expected for the second and third days. There is a fair chance for some isolated storm periods over the next three days.
III. Sündmuste tõenäosus 21 Sepkuni 23 Sep
Klass M20%20%20%
Klass X01%01%01%
Prooton01%01%01%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       20 Sep 112
  Prognoositud   21 Sep-23 Sep  112/115/115
  90 päeva keskmine        20 Sep 120
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 19 Sep  026/032
  Hinnanguline     Afr/Ap 20 Sep  025/025
  Prognoositud    Afr/Ap 21 Sep-23 Sep  020/025-015/020-015/020
VI. Geomagnetilised aktiivsuse tõenäosused 21 Sep kuni 23 Sep
A. Keskmistel laiuskraadidel
Aktiivne40%45%45%
Väike torm25%20%20%
Suur-tõsine torm10%05%05%
B. Kõrgetel laiuskraadidel
Aktiivne25%30%30%
Väike torm35%25%25%
Suur-tõsine torm20%15%10%

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