Vaata laupäev, 29 veebruar 2020 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2020 Feb 29 1231 UTC

SIDC ennustus

Kehtib alates 1230 UTC, 29 Feb 2020 kuni 02 Mar 2020
Päikesepursked ehk loited

Quiet conditions (<50% probability of C-class flares)

Geomagnetism

Active conditions expected (A>=20 or K=4)

Päikese prootonid

Quiet

10 cm voolAp
29 Feb 2020071008
01 Mar 2020071015
02 Mar 2020070012

Bülletään

Solar activity was at very low levels. The Sun remained spotless. STEREO-A/COR2 coronagraphic imagery shows a coronal mass ejection (CME) departing from the Sun's west limb on 28 February (+/- 08UT). This slow CME may have an earth-bound direction, but no related solar disk features or SOHO/LASCO CMEs have been observed to confirm this. If arriving at Earth (around 04 March), at most active geomagnetic conditions are expected. No other earth-directed coronal mass ejections (CMEs) have been observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values. A small and irregularly shaped equatorial negative polarity coronal hole (CH) is present on the solar disk.

Solar activity is expected to remain at very low levels.

Solar wind speed gradually increased from 350 km/s at the beginning of the period to near 500 km/s around 02:45UT, then to decline back to values around 430 km/s by the end of the period (ACE). Bz oscillated between -7 and +7 nT. The direction of the interplanetary magnetic field (phi angle) was predominantly directed away from the Sun until about 18:30UT, when it switched to a mostly negative sector (towards the Sun). These enhanced solar wind streams are most likely related to patchy CHs that were visible on the Sun over the last few days. Geomagnetic conditions were at quiet levels, with an unsettled episode (09-12UT) recorded at Dourbes.

Up to 02 March, geomagnetic activity is expected to be mostly at quiet to unsettled levels, with a chance on an active episode in response to the enhanced wind streams from patchy coronal holes.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 000, põhineb 14 jaamadel.

Päikese indeksid 28 Feb 2020

Catania Wolfi number///
10cm päikesevoog071
AK Chambon La Forêt013
AK Wingst007
Hinnanguline Ap006
Hinnanguline rahvusvaheline päikeselaikude arv000 - Põhineb 28 jaamal

Märkimisväärsete sündmuste kokkuvõte

PäevAlgusMaksLõppLokatsioonTugevusOP10cmCatania/NOAARaadiosignaalipursete tüübid
Puuduvad

Andmed on esitanud Päikeseinfektide Andmeanalüüsi Keskus (Solar Influences Data Analysis Center)© - SIDC - Töötleb SpaceWeatherLive

Kõik ajad UTC-s

<< Mine igapäevase ülevaate lehele

Viimane uudis

Toeta 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!

Anneta SpaceWeatherLive Pro
Toetage SpaceWeatherLive meie kaupadega
Vaadake meie kaupa

Fakte kosmose ilmast

Viimane X-loide28/03/2025X1.1
Viimane M-loide30/04/2025M2.03
Viimane geomagnetiline torm03/05/2025Kp5 (G1)
Plekivabasid päevi
Viimane päikese plekivaba päev08/06/2022
Kuu keskmine päikeseplekkide arv
aprill 2025140.6 +6.4
mai 202558 -82.6
Viimased 30 päeva114 -17.5

See päev ajaloos*

Päikesepursked ehk loited
12000M9.79
22024M9.13
32024M9.1
42022M5.7
52022M5.3
DstG
11998-205G4
21978-152G4
31967-80
41976-55
51983-53G1
*alates 1994

Sotsiaalvõrgustikud