Vaata kolmapäev, 22 aprill 2026 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2026 Apr 22 1231 UTC

SIDC ennustus

Päikesepursked ehk loited

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

Geomagnetism

Quiet (A<20 and K<4)

Päikese prootonid

Quiet

10 cm voolAp
22 Apr 2026118008
23 Apr 2026122008
24 Apr 2026126007

Päikese aktiivsed piirkonnad ja pursked

Solar flaring activity was low over the past 24 hours, with only C-class flares identified. A total of 4 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 825 (NOAA Active Region 4419) and SIDC Sunspot Group 847 (NOAA Active Region 4420) are the largest and most magnetically complex (Beta-Gamma) regions on disk. The largest flare was a C1.9 flare (SIDC Flare 7436) peaking on April 21 at 14:24 UTC, which was produced by SIDC Sunspot Group 847. Solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a chance for M-class flares.

Krooniaine massiline väljavool

A Coronal Mass Ejection (CME) was observed LASCO-C2 data around 23:00 UTC on April 20. This CME is associated with a filament eruption centred around N21, E05, with a speed around 430 km/s. The bulk of the material is expected to travel North and most likely to miss the Earth a glancing blow arrival is possible on April 25 around 09:00 UTC.

Krooniauk

SIDC Coronal Hole 157 (equatorial coronal hole extending to the polar south with a positive polarity) is continuing to cross the central meridian. SIDC Coronal Hole 156 (equatorial coronal hole with a positive polarity) started crossing the central meridian on April 22.

Päikesetuul

Over the past 24 hours the solar wind parameters were under the waning influence of a high-speed stream associated with SIDC Coronal Hole 147. The solar wind speed ranged between 474 km/s to 577 km /s. The total interplanetary magnetic field ranged from 3 to 6 nT, with the Bz reaching a minimum of -5 nT. The phi-angle was mainly in the negative sector (directed towards the Sun), with periods in the positive sector. Quite solar wind conditions are expected in the next 24 hours.

Geomagnetism

The geomagnetic conditions reached active conditions globally (Kp 4) and minor storm conditions locally (K BEL 5) in the last 24 hours. Quiet to unsettled conditions are expected over the next 24 hours.

Prootoni voo tasemed

The greater than 10 MeV GOES proton flux was at background levels and is expected to remain at background levels over the next 24 hours.

Elektronivoog geostatsionaarsel orbiidil

The greater than 2 MeV electron flux, as measured by GOES-18 and GOES-19 was above the 1000 pfu alert threshold in the past 24 hours. The flux is expected to fluctuate around the alert threshold over the next 24 hours. The 24-hour electron fluence was at moderate levels over the past 24 hours and is expected to remain at these levels over the next 24 hours.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 075, põhineb 21 jaamadel.

Päikese indeksid 21 Apr 2026

Catania Wolfi number079
10cm päikesevoog112
AK Chambon La Forêt020
AK Wingst022
Hinnanguline Ap021
Hinnanguline rahvusvaheline päikeselaikude arv056 - Põhineb 32 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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