Vaata esmaspäev, 5 aprill 2021 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2021 Apr 05 1243 UTC

SIDC ennustus

Kehtib alates 1230 UTC, 05 Apr 2021 kuni 07 Apr 2021
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
05 Apr 2021070010
06 Apr 2021070009
07 Apr 2021070004

Bülletään

The solar activity has been quiet over the past 24 hours. Region NOAA 12813 is fading, while two smaller regions in SE have appeared, with no accompanying sunspots. The solar activity has been mostly quiet over the past 24 hours and is expected to remain at low levels over the next 24 hours.

No Earth-directed coronal mass ejections (CMEs) were observed in the available coronagraph imagery.

The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux was at nominal levels, while the greater than 2 MeV electron fluence was at normal levels in the past 24 hours. They are expected to remain at about those levels for the next 24 hours.

Over the past 24 hours the solar wind speed ranged between 280 km/s and 320 km/s. The total magnetic field values were between 0 nT and 9 nT. The Bz component fluctuated between -8 nT and 7 nT. The orientation of the Interplanetary Magnetic Field (IMF) the first part for the last 24-hour window was predominantly to the negative sector (towards the Sun), but has varied during the second half. The solar wind parameters are indicating the beginning of influence from wind emanating from the southern positive Coronal Hole, which was on Central Meridian April 3. As a response, over the next 24 hours the solar wind parameters are expected to increase.

The geomagnetic conditions over the past 24 hours were quiet (Kp: 0-1 and K-Dourbes: 0-2). Quiet to unsettled conditions are expected for the next 24-hour period, with a slight chance of an active event (K Dourbes=4), due to the expected influence of the high-speed stream associated with the equatorial coronal hole (facing Earth on April 3).

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 010, põhineb 13 jaamadel.

Päikese indeksid 04 Apr 2021

Catania Wolfi number///
10cm päikesevoog070
AK Chambon La Forêt006
AK Wingst004
Hinnanguline Ap002
Hinnanguline rahvusvaheline päikeselaikude arv012 - Põhineb 23 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-loide01/04/2025M2.5
Viimane geomagnetiline torm27/03/2025Kp5 (G1)
Plekivabasid päevi
Viimane päikese plekivaba päev08/06/2022
Kuu keskmine päikeseplekkide arv
märts 2025134.2 -20.4
aprill 2025143 +8.8
Viimased 30 päeva130.4 -16.1

See päev ajaloos*

Päikesepursked ehk loited
12002M8.82
21999M6.76
32001M2.91
42003M2.74
52001M2.31
DstG
11979-202G3
21988-133G3
31984-120G4
42004-117G2
51994-111G3
*alates 1994

Sotsiaalvõrgustikud