Vaata esmaspäev, 14 aprill 2003 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 2003 Apr 14 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 104 Välja antud 2200Z kuni 14 Apr 2003IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 13-2100Z kuni 14-2100Z Solar activity was low during the past 24 hours.
Today's only C-class event was a C1 at 0930 UTC from Region 335
(S22E57). Region 334 (S08E29) exhibited the brightest plage
throughout the day but was not able to muster a flare-level event.
Region 330 (N07W57) continues to be the largest group on the disk
but was stable and quiet.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low
for the next three days.
IIA. Summaarne geofüüsikaline aktiivsus 13-2100Z kuni 14-2100Z
The geomagnetic field ranged from quiet to active levels, with a
period of minor storm conditions at high latitudes from 1200-1500
UTC. The enhanced activity was associated with an extended interval
of moderately strong (-5 to -10 nT) southward orientation of the
interplanetary magnetic field Bz component between 1100-1500 UTC.
The greater than 2 MeV electron fluxes were high levels early in the
day but dropped below 1000 PFU after 0525 UTC. Solar wind speed and
temperature showed a gradual increasing trend during the last four
hours of the day, which may indicate the beginning of a high speed
solar wind stream associated with a coronal hole.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be generally unsettled with occasional active periods
over the next three days. There is a chance for some isolated storm
periods at high latitudes.
III. Sündmuste tõenäosus 15 Aprkuni 17 Apr
| Klass M | 10% | 10% | 10% |
| Klass X | 01% | 01% | 01% |
| Prooton | 01% | 01% | 01% |
| PCAF | green | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 14 Apr 102 Prognoositud 15 Apr-17 Apr 100/095/095 90 päeva keskmine 14 Apr 128
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 13 Apr 008/010 Hinnanguline Afr/Ap 14 Apr 015/015 Prognoositud Afr/Ap 15 Apr-17 Apr 012/015-012/015-015/015
VI. Geomagnetilised aktiivsuse tõenäosused 15 Apr kuni 17 Apr
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 40% | 40% | 45% |
| Väike torm | 20% | 20% | 25% |
| Suur-tõsine torm | 05% | 05% | 10% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 35% | 35% | 40% |
| Väike torm | 25% | 25% | 30% |
| Suur-tõsine torm | 05% | 05% | 15% |
<< Mine igapäevase ülevaate lehele
Viimane uudis
laupäev, 23 märts 2024
X1.1 solar flare with earth-directed CME
kolmapäev, 20 märts 2024
Sunspot region 3615, G1 watch
neljapäev, 22 veebruar 2024
X6.3 solar flare
Viimane foorumi postitus
Unspecified geomagnetic activity 904Growth of Cycle 25 417GONG Farside Images added to the SWL site? 3Changelog/Featurelog 152Imagery from Total Solar Eclipse 08/04/2024 5
Veel teemasidToeta 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!
Fakte kosmose ilmast
| Viimane X-loide | 28/03/2024 | X1.1 |
| Viimane M-loide | 19/04/2024 | M1.0 |
| Viimane geomagnetiline torm | 16/04/2024 | Kp5 (G1) |
| Plekivabasid päevi | |
|---|---|
| Viimane päikese plekivaba päev | 08/06/2022 |
| Kuu keskmine päikeseplekkide arv | |
|---|---|
| märts 2024 | 104.9 -19.8 |