Vaata reede, 4 november 2011 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 2011 Nov 04 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 308 Välja antud 2200Z kuni 04 Nov 2011

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 03-2100Z kuni 04-2100Z

Solar activity was moderate. Region 1339 (N19E45) produced two M-class flares during the past 24 hours; an M2 at 03/2336Z and an M1/Sf at 04/2040Z. Region 1339 continues to dominate the disk in terms of sunspot area (about 1540 millionths) and complexity (Fkc beta-gamma-delta). The region did not show a strong growth or decay trend. A fast, asymmetric full halo CME was observed to enter the LASCO C2 field of view at 03/2312Z and had an estimated plane of sky speed of about 1100 km/s. Observations from the STEREO spacecraft indicate this was a back-sided event. An additional CME was observed in the C2 coronagraph at 04/0248Z off the east limb. STEREO-B coronagraph observations appeared to show this as a full halo CME and post-eruption loops were visible extending above the east limb in the GOES SXI imagery. These observations suggest a source that is just behind the east limb. Region 1338 (S14E28) continues to be of moderate size (about 240 millionths) but was quiet and stable.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be moderate. Additional M-flares are likely with Region 1339 as the most probable source although the region behind east limb could also contribute. There is a slight chance for an additional major flare event from Region 1339.
IIA. Summaarne geofüüsikaline aktiivsus 03-2100Z kuni 04-2100Z
The geomagnetic field was quiet. A proton enhancement was observed at the GOES satellites, beginning at about 0100Z and rising to a peak of 3.6 PFU (greater than 10 MeV) at 0905Z. The flux levels slowed decreased thereafter.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be quiet to unsettled for the next two days (05-06 November). A slight increase in activity is predicted due to a small but favorably positioned coronal hole. Quiet levels are expected to prevail for the third day (07 November).
III. Sündmuste tõenäosus 05 Novkuni 07 Nov
Klass M65%65%65%
Klass X10%10%10%
Prooton05%05%10%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       04 Nov 164
  Prognoositud   05 Nov-07 Nov  165/165/170
  90 päeva keskmine        04 Nov 126
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 03 Nov  003/003
  Hinnanguline     Afr/Ap 04 Nov  007/008
  Prognoositud    Afr/Ap 05 Nov-07 Nov  007/010-007/008-005/005
VI. Geomagnetilised aktiivsuse tõenäosused 05 Nov kuni 07 Nov
A. Keskmistel laiuskraadidel
Aktiivne20%15%05%
Väike torm05%01%01%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne25%20%10%
Väike torm15%10%05%
Suur-tõsine torm05%01%01%

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