Vaata teisipäev, 25 mai 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 May 25 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 146 Välja antud 2200Z kuni 25 May 2004IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 24-2100Z kuni 25-2100Z Solar activity was at low levels. Region 615 (N17W53)
produced the largest flare of the period, a C1 x-ray event that
occurred at 24/2239Z. Region 618 (S10W00) was limited to B-class
flare production this period while two delta structures remain
evident across the magnetic region center in this beta-gamma-delta
complex. Little change was noted in sunspot area today. A 20
degree filament that was seen near the north-center of the disk
became active just before 24/1800Z, and had fully erupted by
24/1930Z. This disappearing filament resulted in a northward
directed CME as seen on LASCO imagery and appears to have little
geoeffective potential. No new regions were numbered today.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at
low to moderate levels. Region 618 remains capable of producing
isolated M-class flare activity.
IIA. Summaarne geofüüsikaline aktiivsus 24-2100Z kuni 25-2100Z
The geomagnetic field was at quiet to unsettled levels.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be at quiet to unsettled levels throughout the period.
NOTE: The ACE spacecraft orbit will bring ACE nearly in line with
the Sun from about May 30 to June 2, 2004. During that time solar
radio noise is expected to interfere with spacecraft telemetry
resulting in the loss of solar wind plasma, magnetic field, and
particle data.
III. Sündmuste tõenäosus 26 Maykuni 28 May
| Klass M | 50% | 50% | 50% |
| Klass X | 10% | 10% | 10% |
| Prooton | 05% | 05% | 05% |
| PCAF | green | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 25 May 102 Prognoositud 26 May-28 May 100/100/105 90 päeva keskmine 25 May 105
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 24 May 008/011 Hinnanguline Afr/Ap 25 May 007/010 Prognoositud Afr/Ap 26 May-28 May 007/010-010/010-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 26 May kuni 28 May
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 20% | 20% |
| Väike torm | 05% | 10% | 10% |
| Suur-tõsine torm | 05% | 05% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 20% | 20% | 20% |
| Väike torm | 10% | 10% | 10% |
| Suur-tõsine torm | 05% | 05% | 05% |
Kõik ajad UTC-s
<< Mine igapäevase ülevaate lehele
Viimane uudis
teisipäev, 14 mai 2024
X8.7 solar flare
esmaspäev, 13 mai 2024
M6.6 solar flare with earth-directed CME
pühapäev, 12 mai 2024
Small CME impact, Record visitor amount
Viimane foorumi postitus
Is a long hot summer on the horizon..? ? 2Contender for 3664 arriving? 3AR3664 1037Space Weather Memes 358That was close..? 40
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 |