Vaata teisipäev, 15 juuli 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 Jul 15 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 196 Välja antud 2200Z kuni 15 Jul 2003

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 14-2100Z kuni 15-2100Z

Solar activity was low. Today's activity consisted of a few low-level C-class flares from Region 409 (N15E41). Region 409 showed growth with the development of new spots in the trailing portion of the region. The penumbra in the region has developed to form a compact distribution of spots, suggesting that a delta configuration may form if the current trend continues. A seven degree filament near (N41E11) disappeared between 1046 UTC and 1211 UTC. New Region 411 (N16E62) was assigned today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low to moderate over the next three days, with Region 409 as the most likely source of M-class flares. There is a slight chance for major flare activity from Region 409 if the current trend continues.
IIA. Summaarne geofüüsikaline aktiivsus 14-2100Z kuni 15-2100Z
The geomagnetic field ranged from unsettled to minor storm levels. An initially active geomagnetic field reached minor storm levels from 0000-0600 UTC. Active to minor storm levels were also observed between 0900-1200 UTC. Conditions have been unsettled since 1200 UTC. The activity increase was seen in response to a jump in solar wind velocity and density accompanied by a southward turning of Bz between 14/2100 UTC and 15/0100 UTC. Solar wind conditions remained elevated for the remainder of the day, ranging mostly between 550 to 600 km/s. The solar wind data appear to be consistent with a brief interval of a co-rotating interaction region followed by a high-speed, coronal-hole-driven solar wind stream. The greater than 2 MeV electron flux reached high levels during the past 24 hours.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be active, with a chance for isolated minor storm periods, during the next 24 hours as a solar coronal hole rotates through a geoeffective position. A decline to unsettled to active levels is expected on the second day and a return to mostly unsettled levels is expected by the third day.
III. Sündmuste tõenäosus 16 Julkuni 18 Jul
Klass M40%40%40%
Klass X10%10%10%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       15 Jul 126
  Prognoositud   16 Jul-18 Jul  125/123/121
  90 päeva keskmine        15 Jul 126
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 14 Jul  013/015
  Hinnanguline     Afr/Ap 15 Jul  020/025
  Prognoositud    Afr/Ap 16 Jul-18 Jul  020/025-015/020-010/015
VI. Geomagnetilised aktiivsuse tõenäosused 16 Jul kuni 18 Jul
A. Keskmistel laiuskraadidel
Aktiivne50%40%30%
Väike torm25%20%15%
Suur-tõsine torm05%05%05%
B. Kõrgetel laiuskraadidel
Aktiivne30%30%30%
Väike torm35%25%20%
Suur-tõsine torm20%15%10%

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