Vaata teisipäev, 4 september 2001 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 2001 Sep 04 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 247 Välja antud 2200Z kuni 04 Sep 2001

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

Solar activity was moderate. A gradual rise in X-rays began at around 04/1000Z and continued through the end of this period. Since 04/1500Z, the X-ray baseline ranged from C4 - C8 with occasional fluctuations to the M1 level. Development within regions near the SE limb, the SW limb and within Region 9601 (N13W22) are the likely sources of the enhanced X-rays. Region 9606 (S17E45) produced an impulsive M1/1n at 04/2017Z. Region 9601, at almost 800 millionths of white light area is moderately complex and the largest region on the visible disk. Several plage fluctuations were observed in this region, but only minor C-class flareS were observed. The two M-class flares observed yesterday at 03/1545Z and 03/1841Z were likely associated with CMEs off the SE limb. New region 9607 (S16E68) was numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at moderate to high levels. New regions near the SE limb and developing regions near the SW limb have potential for isolated M-class flares. Region 9601 also has potential for M-class flares.
IIA. Summaarne geofüüsikaline aktiivsus 03-2100Z kuni 04-2100Z
The geomagnetic field was mostly at unsettled to active levels. A high speed coronal hole stream and possibly some weak CME effects are producing the disturbed conditions.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to return to quiet to unsettled conditions by the end of day one and persist through days two and three.
III. Sündmuste tõenäosus 05 Sepkuni 07 Sep
Klass M70%70%70%
Klass X15%15%15%
Prooton15%15%15%
PCAFyellow
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       04 Sep 218
  Prognoositud   05 Sep-07 Sep  210/210/205
  90 päeva keskmine        04 Sep 158
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 03 Sep  012/017
  Hinnanguline     Afr/Ap 04 Sep  015/018
  Prognoositud    Afr/Ap 05 Sep-07 Sep  010/012-010/010-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 05 Sep kuni 07 Sep
A. Keskmistel laiuskraadidel
Aktiivne30%20%20%
Väike torm10%05%05%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne40%25%25%
Väike torm15%05%05%
Suur-tõsine torm05%01%01%

<< 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-loide02/05/2024M1.0
Viimane geomagnetiline torm26/04/2024Kp5+ (G1)
Plekivabasid päevi
Viimane päikese plekivaba päev08/06/2022
Kuu keskmine päikeseplekkide arv
aprill 2024136.5 +31.6
Viimased 30 päeva146.6 +47.6

See päev ajaloos*

Päikesepursked ehk loited
11998X1.61
22000M4.1
32001M2.57
42013M1.61
52003M1.49
ApG
1197660G4
2197894G3
3195168G3
4199863G3
5199449G3
*alates 1994

Sotsiaalvõrgustikud