Vaata kolmapäev, 14 märts 2012 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 2012 Mar 14 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 074 Välja antud 2200Z kuni 14 Mar 2012

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 13-2100Z kuni 14-2100Z

Solar activity was moderate. Region 1432 (N14E03) produced an M2/1N event at 14/1521Z associated with a faint CME as visible on LASCO C2 (plane-of-sky velocity 392 km/s) with a narrow northeast trajectory. As of current, this CME is not expected to be geoeffective.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low to moderate with a slight chance for an isolated X-class flare until Region 1429 (N19W77) rotates behind the limb. On days 2 and 3 (16-17 March) activity is expected to decrease to low levels with a chance for moderate flaring from Region 1432.
IIA. Summaarne geofüüsikaline aktiivsus 13-2100Z kuni 14-2100Z
The geomagnetic field was at quiet to unsettled levels reaching active levels at high latitudes. Correction to yesterdays summary, the greater than 100 MeV event began at 13/1810Z, reached a peak value of 1 PFU at 13/1905Z, and ended at 13/2255Z. The 10 MeV proton event greater than 100 PFU (S2-Moderate) event began at 13/1855Z, reached a peak value of 469 PFU at 13/2045Z, and dropped below 100 PFU into S1-Minor threshold at 14/0955Z. The proton event is currently around 33 PFU and gradually decreasing. The greater than 2 MeV electron flux at geosynchronous orbit was at high levels throughout the period.
IIB. Geofüüsikalise aktiivsuse ennustus
Geomagnetic activity is expected to be quiet to unsettled on 15 March. Activity is expected to increase to active levels on 16 March due to effects from the 13 March transient and a recurrent coronal hole high speed stream. Activity is expected to return to mostly unsettled levels on 17 March as effects from these two influences begin to wane slightly. The greater than 10 MeV proton event is expected to continue to decrease over the next three days.
III. Sündmuste tõenäosus 15 Markuni 17 Mar
Klass M70%40%40%
Klass X20%05%05%
Prooton90%40%70%
PCAFred
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       14 Mar 119
  Prognoositud   15 Mar-17 Mar  115/110/105
  90 päeva keskmine        14 Mar 125
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 13 Mar  010/011
  Hinnanguline     Afr/Ap 14 Mar  006/008
  Prognoositud    Afr/Ap 15 Mar-17 Mar  009/015-015/020-018/015
VI. Geomagnetilised aktiivsuse tõenäosused 15 Mar kuni 17 Mar
A. Keskmistel laiuskraadidel
Aktiivne15%25%25%
Väike torm05%05%10%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne15%20%15%
Väike torm15%30%20%
Suur-tõsine torm05%35%20%

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