Vaata laupäev, 25 juuni 2022 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2022 Jun 25 1231 UTC

SIDC ennustus

Kehtib alates 1230 UTC, 25 Jun 2022 kuni 27 Jun 2022
Päikesepursked ehk loited

C-class flares expected, (probability >=50%)

Geomagnetism

Quiet (A<20 and K<4)

Päikese prootonid

Quiet

10 cm voolAp
25 Jun 2022115010
26 Jun 2022115012
27 Jun 2022115011

Bülletään

The solar flaring activity was at low levels over the past 24 hours with only very few small C-class flares from several sunspots groups visible on the disc seen from Earth. We expect a very low flaring activity with a small chance of isolated C-class flares.

No Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images over the past 24 hours.

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux was below 1000 pfu alert threshold and it is expected to remain so during the next 24 hours. The electron fluence was at normal to moderate levels and is expected to remain normal to moderated levels in the next 24 hours.

The solar wind parameters in Earth environment were showing a slow solar wind-speed regime: the wind speed ranged between 354 km/s and 462 km/s. The interplanetary magnetic field magnitude showed some higher values with an increase from 5 nT in the beginning of the periods to the current values aournd 13 nT. The Bz component of the interplanetary magnetic field fluctuated between -8.3 nT and 10.4 nT being predominately negative. The high-speed streams coming from the coronal holes (negative polarity) may influence the solar wind conditions and contribute to its enhancement in next days.

The geomagnetic conditions were mostly quiet to unsettle (NOAA Kp and local K-Belgium 1-3). An isolated period of active conditions (K-Belgium = 4) was observed from local stations in Belgium in responses to the prolonged negative values of the Bz component of the interplanetary magnetic field. The geomagnetic conditions are expected to be mostly quiet to unsettle with possible periods of active conditions in responses to the prolonged negative values of the Bz component.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 052, põhineb 19 jaamadel.

Päikese indeksid 24 Jun 2022

Catania Wolfi number///
10cm päikesevoog115
AK Chambon La Forêt016
AK Wingst010
Hinnanguline Ap011
Hinnanguline rahvusvaheline päikeselaikude arv069 - Põhineb 21 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

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