Vaata pühapäev, 22 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 22 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 173 Välja antud 2200Z kuni 22 Jun 2003

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 21-2100Z kuni 22-2100Z

Solar activity was low. Just a single C-class flare this period - a C1/Sf at 22/0949Z from Region 388 (S02W32). This region has shown little change this period and still contains some weak magnetic mixing. Moderately complex Region 386 (S06W08) still maintains a weak delta configuration, but was quiet this period as it continues to slowly decay. Region 387 (N18E10) is the largest region the visible disk, but was also quiet. A new region rotating around the east limb was numbered today as Region 390.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to continue at low levels. There is a small chance for an isolated low M-class flare from Regions 386, 387 and 388.
IIA. Summaarne geofüüsikaline aktiivsus 21-2100Z kuni 22-2100Z
The geomagnetic field was unsettled to active due to a high speed coronal hole stream. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to continue at unsettled to active levels due to coronal hole high speed flow.
III. Sündmuste tõenäosus 23 Junkuni 25 Jun
Klass M25%25%25%
Klass X05%05%05%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       22 Jun 110
  Prognoositud   23 Jun-25 Jun  110/115/115
  90 päeva keskmine        22 Jun 126
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 21 Jun  016/023
  Hinnanguline     Afr/Ap 22 Jun  015/015
  Prognoositud    Afr/Ap 23 Jun-25 Jun  015/015-012/012-012/012
VI. Geomagnetilised aktiivsuse tõenäosused 23 Jun kuni 25 Jun
A. Keskmistel laiuskraadidel
Aktiivne35%30%30%
Väike torm15%10%10%
Suur-tõsine torm05%05%05%
B. Kõrgetel laiuskraadidel
Aktiivne40%35%35%
Väike torm20%15%15%
Suur-tõsine torm10%05%05%
Comments K-Indices On 16 June, it was determined that a scaling problem exists with the Boulder magnetometer instrument. While this problem, and its fix are being investigated, the primary instrument for Boulder K-indices has been switched to the Boulder USGS (via Domsat) magnetometer, effective 1500 UTC on 16 June. GOES Protons To ensure continued operational monitoring of important energetic particle data, it is necessary to reassign primary/secondary designations for the GOES Space Environment Monitor (SEM) detectors. GOES 11 (113W) is now the primary satellite for protons. GOES 12 will continue as the primary satellite for magnetometer, X-ray, and electron measurements. GOES 10 (135W) will be the secondary satellite for all SEM sensors - magnetometer, X-ray, and energetic particles. Because of the degraded state of the proton data on GOES-10, its designation as the secondary source for proton data is a short-term solution. More permanent solutions have been identified and are being evaluated. Users will be notified when we define and schedule a permanent fix. Further details can be found at http://www.sec.noaa.gov/GOES.html.

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