Vaata reede, 1 märts 2002 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 2002 Mar 01 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 060 Välja antud 2200Z kuni 01 Mar 2002

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 28-2100Z kuni 01-2100Z

Solar activity has been low. Several C-class events occurred, the largest being a C9.7 flare at 01/0012 UTC. No corresponding optical flare report was received for this event, but SOHO/EIT imagery suggests that Region 9845 (N17W04) was the source. Two type-II radio sweep events occurred during the period. The first was at 01/0214 UTC, with an estimated velocity of 1200 km/s. SOHO/LASCO imagery revealed a fast CME from a source behind the southwest limb at this time, though not appearing earth-directed. The second sweep had an estimated velocity of 742 km/s and occurred at 01/0542 UTC, shortly after an impulsive C7/Sf from Region 9848 (S20W21) at 01/0531 UTC. However, no CME activity was evident in LASCO imagery following this event. Two new regions were numbered today: 9851 (S07E56), and 9852 (N16E66).
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low to moderate for the next three days. Region 9845 is a possible source for isolated M-class flares.
IIA. Summaarne geofüüsikaline aktiivsus 28-2100Z kuni 01-2100Z
Geomagnetic field activity was at quiet to minor storm levels. A sustained period of southward IMF, following a weak interplanetary shock passage early on 28 February, caused active and isolated minor storm conditions at higher latitudes during 28/2100 - 01/0300 UTC. Activity has been predominantly quiet since then.
IIB. Geofüüsikalise aktiivsuse ennustus
Geomagnetic field activity is expected to be mainly quiet to unsettled, until the onset of high speed stream effects from a recurrent coronal hole begin to develop by day three of the forecast period. Isolated active conditions are anticipated thereafter.
III. Sündmuste tõenäosus 02 Markuni 04 Mar
Klass M40%40%40%
Klass X01%01%01%
Prooton01%01%01%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       01 Mar 188
  Prognoositud   02 Mar-04 Mar  190/190/190
  90 päeva keskmine        01 Mar 223
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 28 Feb  015/017
  Hinnanguline     Afr/Ap 01 Mar  010/010
  Prognoositud    Afr/Ap 02 Mar-04 Mar  005/006-005/008-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 02 Mar kuni 04 Mar
A. Keskmistel laiuskraadidel
Aktiivne15%15%25%
Väike torm05%05%10%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne20%20%30%
Väike torm05%05%10%
Suur-tõsine torm01%01%01%

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