Vaata esmaspäev, 9 veebruar 2004 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 2004 Feb 09 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 040 Välja antud 2200Z kuni 09 Feb 2004IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 08-2100Z kuni 09-2100Z Solar activity decreased to low levels today. Region
554 (S08E52) produced numerous B and C-class flares today. Ten
C-class flares were recorded with the largest being a C9 x-ray event
that occurred at 09/1102Z. LASCO imagery has shown little, if any
associated CME signatures during the past 24 hours of activity from
this region. Magnetic analysis depicts a delta configuration within
the dominant intermediate spot. Region 551 (S06W27) did not manage
any flare production during the interval, although surging and point
brightenings were observed throughout the period. The gamma
structures in the central and trailing portions of the sunspot group
remain intact. Region 555 (S14E72) was numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at
low to moderate levels. Regions 551 and 554 both have the potential
to produce M-class flare activity.
IIA. Summaarne geofüüsikaline aktiivsus 08-2100Z kuni 09-2100Z
The geomagnetic field was at quiet to unsettled levels. The greater
than 2 MeV electron fluxes at geosynchronous orbit reached high
levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be at quiet to unsettled levels. 12 February may
experience active conditions due to a solar sector boundary
crossing, preceding an anticipated recurrent high speed coronal hole
stream.
III. Sündmuste tõenäosus 10 Febkuni 12 Feb
| Klass M | 50% | 50% | 50% |
| Klass X | 15% | 15% | 15% |
| Prooton | 05% | 05% | 05% |
| PCAF | green | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 09 Feb 118 Prognoositud 10 Feb-12 Feb 120/120/115 90 päeva keskmine 09 Feb 121
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 08 Feb 002/008 Hinnanguline Afr/Ap 09 Feb 004/009 Prognoositud Afr/Ap 10 Feb-12 Feb 006/010-008/012-012/015
VI. Geomagnetilised aktiivsuse tõenäosused 10 Feb kuni 12 Feb
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 10% | 15% | 20% |
| Väike torm | 05% | 05% | 10% |
| Suur-tõsine torm | 01% | 01% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 20% | 30% |
| Väike torm | 05% | 10% | 15% |
| Suur-tõsine torm | 01% | 05% | 05% |
Kõik ajad UTC-s
<< Mine igapäevase ülevaate lehele
Viimane uudis
kolmapäev, 15 mai 2024
More X-flares!
teisipäev, 14 mai 2024
X8.7 solar flare
esmaspäev, 13 mai 2024
M6.6 solar flare with earth-directed CME
Viimane foorumi postitus
May 2024 Geomagnetic Storms from AR 13664 (2) 303Trying to identify if this is STEVE? 9Incoming Active Regions 334Unproven theories 445AR3664 1048
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 | 15/05/2024 | X2.9 |
| Viimane M-loide | 15/05/2024 | M3.2 |
| Viimane geomagnetiline torm | 13/05/2024 | Kp6 (G2) |
| Plekivabasid päevi | |
|---|---|
| Viimane päikese plekivaba päev | 08/06/2022 |
| Kuu keskmine päikeseplekkide arv | |
|---|---|
| aprill 2024 | 136.5 +31.6 |
| mai 2024 | 151.7 +15.2 |
| Viimased 30 päeva | 176.8 +77.8 |