Vaata neljapäev, 6 november 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 Nov 06 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 310 Välja antud 2200Z kuni 06 Nov 2003IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 05-2100Z kuni 06-2100Z Solar activity was at very low levels. After nearly
three weeks of intense solar activity, the visible surface of the
sun is almost spotless. Region 495 (S21W76) is the only spot group
visible and has exhibited little change from yesterday. A long
duration B5 X-ray enhancement was observed at 06/1831Z and EIT
imagery suggests a source from beyond the west limb.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to range
from very low to low.
IIA. Summaarne geofüüsikaline aktiivsus 05-2100Z kuni 06-2100Z
The geomagnetic field was at quiet to minor storm levels. The shock
from the X28 flare on 04 November reached Earth at 06/1937Z. A 31nT
sudden impulse was observed on the Boulder magnetometer and activity
reached minor storm levels. The Bz component of the interplanetary
magnetic field, as measured by the NASA/ACE spacecraft initially
turned south to -7 nT and total field measurement reached 15 nT. A
greater than 10 MeV proton event continues with current flux levels
at 18 pfu and slowly decreasing.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be at quiet to active levels with isolated minor storm
levels possible. Active levels with isolated minor storm levels are
expected on day one. By day two and three activity is expected to
return to quiet to unsettled levels. The greater than 10 MeV proton
event is expected to end early on day one.
III. Sündmuste tõenäosus 07 Novkuni 09 Nov
| Klass M | 10% | 01% | 01% |
| Klass X | 01% | 01% | 01% |
| Prooton | 50% | 10% | 05% |
| PCAF | in progress | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 06 Nov 098 Prognoositud 07 Nov-09 Nov 095/090/090 90 päeva keskmine 06 Nov 131
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 05 Nov 004/009 Hinnanguline Afr/Ap 06 Nov 012/015 Prognoositud Afr/Ap 07 Nov-09 Nov 020/020-010/015-015/015
VI. Geomagnetilised aktiivsuse tõenäosused 07 Nov kuni 09 Nov
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 35% | 20% | 25% |
| Väike torm | 20% | 10% | 10% |
| Suur-tõsine torm | 10% | 05% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 45% | 25% | 25% |
| Väike torm | 35% | 15% | 15% |
| Suur-tõsine torm | 20% | 10% | 10% |
<< Mine igapäevase ülevaate lehele
Viimane uudis
laupäev, 4 mai 2024
Sunspot region 3663, X1 solar flare
esmaspäev, 22 aprill 2024
Lot's of sunspots! Big chance for major flare activity?
laupäev, 23 märts 2024
X1.1 solar flare with earth-directed CME
Viimane foorumi postitus
2024/05/03 X1.69 CME 28AR3664 37Space Weather Memes 345AR3663 207CME Imagery isn't updating since May 3rd. 8
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 | 06/05/2024 | X4.4 |
| Viimane M-loide | 06/05/2024 | M1.5 |
| Viimane geomagnetiline torm | 02/05/2024 | Kp7- (G3) |
| Plekivabasid päevi | |
|---|---|
| Viimane päikese plekivaba päev | 08/06/2022 |
| Kuu keskmine päikeseplekkide arv | |
|---|---|
| aprill 2024 | 136.5 +31.6 |
| Viimased 30 päeva | 156.6 +63.6 |