Vaata kolmapäev, 28 juuli 2004 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 2004 Jul 28 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 210 Välja antud 2200Z kuni 28 Jul 2004

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 27-2100Z kuni 28-2100Z

Solar activity has declined to low levels. Region 652 (N08W76) continues to be quite active and produced several C-class events this period. The most important was a very long duration C4 enhancement that began around 28/0200Z and lasted for 10 hours. LASCO imagery showed a large CME off the west limb originating from near Region 652. Though most of the ejecta was westward directed, a glancing blow is possible from this CME. Region 652 continues to slowly decay, but still maintains considerable size and magnetic complexity. No other significant changes were noted.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be very low to moderate. Region 652 still has potential for an M-class flare before it rotates around the west limb on 29 July. Expect levels to decrease to very low to low by 30 July.
IIA. Summaarne geofüüsikaline aktiivsus 27-2100Z kuni 28-2100Z
The geomagnetic field ranged from quiet to minor storm levels. The period began with minor storm levels in the waning stages of yesterday's severe geomagnetic storm. By 28/0300Z, the IMF Bz was near zero and the geomagnetic field responded with quiet to unsettled conditions for the remainder of the period. Solar wind speed was elevated near 900 km/s at the beginning of the period, but gradually declined to 600 km/s. The greater than 10 MeV proton event that began on 25/1855Z, ended on 28/0040Z. The greater than 2 MeV electron flux at geosynchronous orbit was at very high levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be quiet to unsettled on 29 July. Today's CME off the southwest limb is expected to produce unsettled to minor storm periods late on 30 July. A gradual return to quiet to unsettled conditions is expected on 31 July.
III. Sündmuste tõenäosus 29 Julkuni 31 Jul
Klass M40%20%05%
Klass X10%05%01%
Prooton15%05%05%
PCAFyellow
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       28 Jul 101
  Prognoositud   29 Jul-31 Jul  090/080/080
  90 päeva keskmine        28 Jul 106
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 27 Jul  119/162
  Hinnanguline     Afr/Ap 28 Jul  012/015
  Prognoositud    Afr/Ap 29 Jul-31 Jul  012/015-020/030-015/020
VI. Geomagnetilised aktiivsuse tõenäosused 29 Jul kuni 31 Jul
A. Keskmistel laiuskraadidel
Aktiivne25%35%25%
Väike torm10%15%10%
Suur-tõsine torm01%05%05%
B. Kõrgetel laiuskraadidel
Aktiivne30%45%35%
Väike torm15%20%15%
Suur-tõsine torm05%10%05%

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