Vaata teisipäev, 4 juuni 2024 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2024 Jun 04 1231 UTC

SIDC ennustus

Päikesepursked ehk loited

M-class flares expected (probability >=50%)

Geomagnetism

Minor storm expected (A>=30 or K=5)

Päikese prootonid

Quiet

10 cm voolAp
04 Jun 2024190024
05 Jun 2024195007
06 Jun 2024195007

Päikese aktiivsed piirkonnad ja pursked

Solar flaring activity was moderate over the past 24 hours. The largest flare was a M4.8-flare, with peak time 14:11 UTC on June 03 associated with NOAA AR 3695 (beta). There are currently 11 numbered active regions on the visible disk. NOAA AR 3697 is the most complex AR (beta-gamma-delta) and is responsible for the majority of the flaring activity of the last 24h, including the M2.4-flare with peak time 6:31 UTC June 04. The solar flaring activity is expected to be at moderate levels over the coming day with C-class flares expected and M-class flares likely and a chance of X-class flares.

Krooniaine massiline väljavool

No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.

Päikesetuul

The solar wind at the Earth was initially slow, with speeds of 300 km/s and interplanetary magnetic field around 5 nT and Bz reaching minimum value of -5nT. Around 21:00 UTC June 03 the magnetic field went up to 18nT and later on the minimum Bz was -10 nT. The solar wind speed increased slowly from this time on to 400 km/s. A minor increase of the solar wind speed and magnetic field is expected later on June 04, due to the potential arrival of the CME of June 01.

Geomagnetism

Geomagnetic conditions reached minor storm level (NOAA Kp 5, Local K Bel 4) June 03 between 21:00- 24:00 UTC. Geomagnetic conditions may reach active to minor storm conditions in the next 24h due to the possible arrival from the CME of June 01.

Prootoni voo tasemed

Over the past 24 hours, the greater than 10 MeV GOES proton flux remained below the 10 pfu threshold and is expected to remain so over the next day. There is a slight chance that the proton flux may increase due to strong flaring from NOAA AR 3697.

Elektronivoog geostatsionaarsel orbiidil

The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, and is expected to remain below the threshold during the next 24 hours. The 24h electron fluence was at normal levels and is expected to remain so.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 222, põhineb 15 jaamadel.

Päikese indeksid 03 Jun 2024

Catania Wolfi number258
10cm päikesevoog186
AK Chambon La Forêt021
AK Wingst013
Hinnanguline Ap012
Hinnanguline rahvusvaheline päikeselaikude arv215 - Põhineb 21 jaamal

Märkimisväärsete sündmuste kokkuvõte

PäevAlgusMaksLõppLokatsioonTugevusOP10cmCatania/NOAARaadiosignaalipursete tüübid
03121812271231S18W01M2.8SF28/3697
03135814111423N28W42M4.82N27/3695III/2
04060906310651S20W09M2.41N28/3697
04085709040908S19W12M1.6SN28/3697

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

Kõik ajad UTC-s

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