Vaata neljapäev, 20 jaanuar 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 Jan 20 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 020 Välja antud 2200Z kuni 20 Jan 2005

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 19-2100Z kuni 20-2100Z

Solar activity was high. Region 720 (N14W70) produced an X7/2b flare at 0701 UTC, which was accompanied by Type II and Type IV radio sweeps. There is one image from the LASCO C2 coronagraph which shows an associated CME off the northwest limb at 0654 UTC. However, shortly after this observation the coronagraph data became difficult to use due to high levels of energetic particles. Region 720 continues to be large, with a sheared magnetic delta configuration along an east-west polarity inversion line.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be moderate to high. Region 720 continues to have potential for producing an additional major flare. The location of Region 720 on the disk also implies that there is a fair chance for more energetic particles in association with future major flare activity.
IIA. Summaarne geofüüsikaline aktiivsus 19-2100Z kuni 20-2100Z
The geomagnetic field was quiet to active during the past 24 hours. Solar wind speeds were elevated (700-900 km/s) from the start of the interval up through at least 0700 UTC, after which the ACE real-time SWEPAM data became unusable due to elevated energetic particle flux. The interplanetary magnetic field, however, was weak with fluctuations between -4 nT to +6 nT. A new injection of protons was observed at 0650 UTC in association with the X7 flare. The greater than 100 MeV protons rose rapidly and attained a maximum of 652 PFU at 0710 UTC. The 100 MeV flux has been declining steadily since then. This high flux level makes this the largest greater than 100 MeV proton event observed since October 1989. A greater than 10 MeV proton event was in progress at the time of the new injection, but the new particles quickly increased the flux from initial values around 40 PFU to a peak value in the past 24 hours of 1860 PFU at 0810 UTC.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is expected to be predominantly unsettled to active for the next three days. Today's CME (associated with the X7 flare) is not expected to produce anything more than a glancing blow due to its direction away from the Sun-Earth line. The greater than 10 MeV flux is expected to remain above event threshold for at least another 24 hours.
III. Sündmuste tõenäosus 21 Jankuni 23 Jan
Klass M90%90%80%
Klass X30%30%20%
Prooton99%80%50%
PCAFin progress
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       20 Jan 123
  Prognoositud   21 Jan-23 Jan  115/105/095
  90 päeva keskmine        20 Jan 108
V. Geomagneetiline A-indeks
  Vaadeldud Afr/Ap 19 Jan  031/062
  Hinnanguline     Afr/Ap 20 Jan  012/015
  Prognoositud    Afr/Ap 21 Jan-23 Jan  015/025-015/020-010/020
VI. Geomagnetilised aktiivsuse tõenäosused 21 Jan kuni 23 Jan
A. Keskmistel laiuskraadidel
Aktiivne35%35%20%
Väike torm20%20%15%
Suur-tõsine torm15%15%05%
B. Kõrgetel laiuskraadidel
Aktiivne35%35%20%
Väike torm20%20%15%
Suur-tõsine torm15%15%10%

<< 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-loide25/04/2024M1.3
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 päeva136.8 +28.6

See päev ajaloos*

Päikesepursked ehk loited
11998X1.54
22006X1.13
32003M2.46
42001M1.81
52023M1.8
ApG
11956172G4
2195554G4
3193761G3
4196031G3
5199530G2
*alates 1994

Sotsiaalvõrgustikud