Vaata laupäev, 16 september 2000 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 2000 Sep 16 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 260 Välja antud 2200Z kuni 16 SEP 2000

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 15-2100Z kuni 16-2100Z

SOLAR ACTIVITY WAS HIGH. REGION 9165 (N13W14) PRODUCED AN M5/2B AT 16/0426 UTC. THIS FLARE WAS ASSOCIATED WITH TYPE II AND IV SWEEPS AND AN 1100 SFU RADIO BURST AT 2695 MHZ. IN ADDITION, THE LASCO INSTRUMENT ON THE SOHO SPACECRAFT OBSERVED AN EARTH-DIRECTED CME FOLLOWING THIS FLARE. REGION 9165 ALSO PRODUCED AN M3/2N AT 16/1428 UTC AS WELL AS SEVERAL C-CLASS FLARES. THIS REGION REMAINS THE LARGEST AND MOST COMPLEX ON THE VISIBLE DISK BUT HAS SHOWN SOME PENUMBRAL DECAY AND MAGNETIC SIMPLIFICATION SINCE YESTERDAY. REGION 9166 (S14E50) CONTINUED TO GENERATE SMALL C-CLASS FLARES. THIS REGION HAS UNDERGONE SOME GROWTH IN SPOT AREA AND NUMBER SINCE YESTERDAY. NEW REGION 9167 (N12E80) IS ROTATING AROUND THE EAST LIMB.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY IS EXPECTED TO BE MODERATE TO HIGH. REGION 9165 IS THE MOST LIKELY CANDIDATE FOR ENERGETIC FLARE ACTIVITY. IIA. GEOPHYSICAL ACTIVITY SUMMARY 15/2100Z TO 16/2100Z: THE GEOMAGNETIC FIELD WAS QUIET TO ACTIVE. THE BZ COMPONENT OF THE IMF HAS FLUCTUATED BETWEEN 0 AND -10NT FOR ABOUT THE LAST 24 HOURS WHILE WIND SPEED HAS BEEN BELOW 400 KM/S AND DENSITY ABOUT 10 P/CC. THE GREATER THAN 10 MEV PROTON EVENT DROPPED BELOW EVENT THRESHOLD (10 PFU) AT 15/2140 UTC. CURRENT FLUX AT GREATER THAN 10 MEV REMAINS ENHANCED AT ABOUT 5 PFU BUT IS DROPPING SLOWLY.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS EXPECTED TO BE MOSTLY UNSETTLED WITH OCCASIONAL ACTIVE PERIODS FOR THE FIRST TWO DAYS OF THE FORECAST PERIOD. STORM CONDITIONS MAY BEGIN BY THE THIRD DAY DUE TO THE M5/2B FLARE AND RELATED CME THAT OCCURRED EARLY ON SEP 16.
III. Sündmuste tõenäosus 17 SEPkuni 19 SEP
Klass M75%75%75%
Klass X10%10%10%
Prooton05%05%05%
PCAFGREEN
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       16 SEP 175
  Prognoositud   17 SEP-19 SEP  180/185/185
  90 päeva keskmine        16 SEP 176
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 15 SEP  013/010
ESTIMATED AFR/AP 16 SEP  015/017
PREDICTED AFR/AP 17 SEP-19 SEP  015/015-015/012-040/040
VI. Geomagnetilised aktiivsuse tõenäosused 17 SEP kuni 19 SEP
A. Keskmistel laiuskraadidel
Aktiivne30%30%50%
Väike torm15%15%30%
Suur-tõsine torm05%05%15%
B. Kõrgetel laiuskraadidel
Aktiivne30%30%50%
Väike torm15%15%30%
Suur-tõsine torm05%05%15%

<< 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!

23%
Toetage SpaceWeatherLive meie kaupadega
Vaadake meie kaupa

Fakte kosmose ilmast

Viimane X-loide22/02/2024X6.3
Viimane M-loide19/03/2024M1.4
Viimane geomagnetiline torm03/03/2024Kp6- (G2)
Plekivabasid päevi
Viimane päikese plekivaba päev08/06/2022
Kuu keskmine päikeseplekkide arv
veebruar 2024124.7 +1.7

See päev ajaloos*

Päikesepursked ehk loited
12003M5.34
22003M2.33
32000M2.29
42003M2.23
52003M2
ApG
1200137G3
2200638G2
3200219G1
4201526G1
5200511G1
*alates 1994

Sotsiaalvõrgustikud