Vaata pühapäev, 12 detsember 2010 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 2010 Dec 12 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 346 Välja antud 2200Z kuni 12 Dec 2010IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 11-2100Z kuni 12-2100Z Solar activity was very low. A filament eruption
occurred in the southwest quadrant and was first observed in
STEREO-A imagery at about 12/0330Z. Coincident with the eruption was
a long duration B4 x-ray event that peaked at 12/0628Z. During the
past 24 hours, three separate CMEs were observed in LASCO C2
imagery. The first was observed departing the southwest limb at
12/0412Z. Subsequent CMEs were observed departing from the northeast
limb at 12/0524Z and from the southeast limb at 12/0612Z. The
remainder of the disk and limb was largely unchanged.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be very
low, with a slight chance for a C-class event from Region 1131
(N31W58), for the next 3 days (13-15 December).
IIA. Summaarne geofüüsikaline aktiivsus 11-2100Z kuni 12-2100Z
The geomagnetic field was predominantly quiet. At approximately
12/1500Z, the field became unsettled to active in response to the
arrival of a coronal hole high speed stream.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to remain quiet to unsettled, with isolated active periods,
for Day 1 (13 December). A return to mostly quiet conditions is
expected for Days 2 and 3 (14-15 December) as the coronal hole high
speed stream departs. At this time, the three CMEs observed in the
past 24 hours are not expected to be geoeffective.
III. Sündmuste tõenäosus 13 Deckuni 15 Dec
| Klass M | 01% | 01% | 01% |
| Klass X | 01% | 01% | 01% |
| Prooton | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 12 Dec 089 Prognoositud 13 Dec-15 Dec 090/090/088 90 päeva keskmine 12 Dec 083
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 11 Dec 001/001 Hinnanguline Afr/Ap 12 Dec 005/005 Prognoositud Afr/Ap 13 Dec-15 Dec 007/010-005/008-005/008
VI. Geomagnetilised aktiivsuse tõenäosused 13 Dec kuni 15 Dec
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 10% | 05% |
| Väike torm | 01% | 01% | 01% |
| Suur-tõsine torm | 01% | 01% | 01% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 20% | 10% | 05% |
| Väike torm | 05% | 01% | 01% |
| Suur-tõsine torm | 01% | 01% | 01% |
<< Mine igapäevase ülevaate lehele
Viimane uudis
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
kolmapäev, 20 märts 2024
Sunspot region 3615, G1 watch
Viimane foorumi postitus
Unspecified geomagnetic activity 990ionosphere D detection 17CME 2024-MAY-01 south of AR3654 C5.8 5AR3663 17Minor glitch with utc timestamp 3
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 | 02/05/2024 | M1.0 |
| Viimane geomagnetiline torm | 26/04/2024 | Kp5+ (G1) |
| Plekivabasid päevi | |
|---|---|
| Viimane päikese plekivaba päev | 08/06/2022 |
| Kuu keskmine päikeseplekkide arv | |
|---|---|
| aprill 2024 | 136.5 +31.6 |
| Viimased 30 päeva | 146.6 +47.6 |