Vaata kolmapäev, 8 juuni 2005 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 2005 Jun 08 2210 UTC
# Prepared jointly by the U.S. Dept. of Commerce, NOAA, #Space Environment Center and the U.S. Air Force. #

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 159 Välja antud 2200Z kuni 08 Jun 2005

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 07-2100Z kuni 08-2100Z

Solar activity was at low levels. Region 776 (S06E33) produced multiple B and C-class flares today. The largest was a C2 x-ray flare that occurred at 08/0625Z. There was some visible growth seen in sunspot area. Region 775 (N10E21) underwent growth in two of the satellite sunspots which now appear to be attached to the dominant central sunspot. Magnetic analysis indicates this region to have beta-gamma-delta characteristics. Region 772 (S18W58) was limited to minor B-class flare production while showing a slight growth in sunspot area. A partial halo CME was observed on LASCO imagery beginning at 08/0512Z which is slow moving and appears to have an Earth directed component. The source for the activity appears to be related to a disappearing solar filament just to the northwest of Region 772. The remaining active regions were quiescent during the period. No new regions were numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at low levels. Regions 775 and 776 both have the potential of producing isolated M-class flares.
IIA. Summaarne geofüüsikaline aktiivsus 07-2100Z kuni 08-2100Z
The geomagnetic field was at quiet to unsettled levels. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be at quiet to unsettled levels throughout the period. There is a slight chance that the effects of the partial halo CME that occurred today could begin to be felt late on day three (11 July).
III. Sündmuste tõenäosus 09 Junkuni 11 Jun
Klass M25%25%25%
Klass X05%05%05%
Prooton05%05%05%
PCAFgreen
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       08 Jun 116
  Prognoositud   09 Jun-11 Jun  115/115/110
  90 päeva keskmine        08 Jun 094
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 07 Jun  011/018
  Hinnanguline     Afr/Ap 08 Jun  005/007
  Prognoositud    Afr/Ap 09 Jun-11 Jun  006/008-006/008-010/008
VI. Geomagnetilised aktiivsuse tõenäosused 09 Jun kuni 11 Jun
A. Keskmistel laiuskraadidel
Aktiivne15%15%25%
Väike torm05%05%10%
Suur-tõsine torm01%01%05%
B. Kõrgetel laiuskraadidel
Aktiivne20%20%25%
Väike torm05%05%10%
Suur-tõsine torm01%01%05%

<< Mine igapäevase ülevaate lehele

Viimane uudis

Toeta SpaceWeatherLive.com-i!

Paljud inimesed külastavad SpaceWeatherLive lehte selleks, et jälgida, mis toimub Päikesel või, kas on oodata virmalisi. Suurema liiklusega on serveri koormus ning maksumus kõrgem. Kui sulle meeldib see, mida me sinu heaks teeme, siis saad sa sellele ka ise natukene kaasa aidata, annetades selle lehe käigus hoidmise ja arendamise heaks. Ette tänades SpeaceWeatherLive meeskond!

54%
Toetage SpaceWeatherLive meie kaupadega
Vaadake meie kaupa

Fakte kosmose ilmast

Viimane X-loide28/03/2024X1.1
Viimane M-loide29/04/2024M3.6
Viimane geomagnetiline torm26/04/2024Kp5+ (G1)
Plekivabasid päevi
Viimane päikese plekivaba päev08/06/2022
Kuu keskmine päikeseplekkide arv
märts 2024104.9 -19.8
Viimased 30 päeva139 +32.6

See päev ajaloos*

Päikesepursked ehk loited
11998M9.27
22024M3.6
32024M2.5
41999M1.7
52003M1.69
ApG
1195658G4
2195287G3
3199159G3
4196055G2
5197359G2
*alates 1994

Sotsiaalvõrgustikud