Vaata kolmapäev, 3 november 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 Nov 03 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 03 Nov 2004

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 02-2100Z kuni 03-2100Z

Solar activity was high during the last 24 hours due to an M5/Sn flare from Region 696 (N09E32) at 1547 UTC. The flare was accompanied by type II and type IV radio sweeps, strong radio bursts, and an asymmetric halo CME with plane-of-sky velocity of about 900 km/s. The majority of the CME mass was observed over the northeast limb. Region 696 produced additional M-flares including an M1/1n at 0335 UTC (accompanied by type II and type IV sweeps and a bright, partial halo CME off the northeast limb), and an M1/Sf at 1826 UTC. The region has more than doubled in size, and of particular note is the emergence of positive polarity magnetic flux just ahead of the strong, negative polarity leader spots. The magnetic inversion between these parts of the group is driving the increased flare production and is close to becoming a magnetic delta configuration. Region 691 (N13W81) started producing flares again after a quiet day yesterday, including an M2/1f at 0133 UTC which was accompanied by a type II sweep. Region 693 (S15W18) continues to be the largest group on the disk but only managed to produce a C2/Sf at 0931 UTC. There is some negative polarity flux emerging in the positive polarity trailer which could trigger more frequent flare activity out of this region.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be moderate, but there is a fair chance for an isolated major flare event over the next three days from Region 696, Region 691, or Region 693.
IIA. Summaarne geofüüsikaline aktiivsus 02-2100Z kuni 03-2100Z
The geomagnetic field was mostly quiet to unsettled during the past 24 hours. There was one active period from 0900-1200 UTC.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be mostly unsettled with possible active periods for the next two days (04-05 November) due to coronal hole effects. The CME associated with today's M5 flare is expected to arrive on the third day (06 November) and is expected to increase activity to mostly active levels with occasional periods of minor storm levels.
III. Sündmuste tõenäosus 04 Novkuni 06 Nov
Klass M65%65%55%
Klass X20%20%15%
Prooton20%20%15%
PCAFyellow
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       03 Nov 136
  Prognoositud   04 Nov-06 Nov  135/130/130
  90 päeva keskmine        03 Nov 108
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 02 Nov  002/004
  Hinnanguline     Afr/Ap 03 Nov  005/007
  Prognoositud    Afr/Ap 04 Nov-06 Nov  012/015-012/015-025/030
VI. Geomagnetilised aktiivsuse tõenäosused 04 Nov kuni 06 Nov
A. Keskmistel laiuskraadidel
Aktiivne25%25%35%
Väike torm15%15%25%
Suur-tõsine torm05%05%15%
B. Kõrgetel laiuskraadidel
Aktiivne30%30%25%
Väike torm15%15%35%
Suur-tõsine torm10%10%25%

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