Vaata teisipäev, 20 veebruar 2024 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2024 Feb 20 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
20 Feb 2024148008
21 Feb 2024146010
22 Feb 2024144010

Päikese aktiivsed piirkonnad ja pursked

Solar flaring activity over the past 24 hours was at low levels. The largest flare was a C5.7-flare, with peak time 12:47 UTC on February 19, associated with NOAA AR 3590 (beta-gamma). There are currently 5 numbered active regions on the visible disk. NOAA AR 3590 (beta-gamma), NOAA AR 3586 (beta) and NOAA AR 3583 (beta) are the most magnetically complex region. NOAA AR 3583 are NOAA AR 3581 (alfa) are rotating over the west limb. All other regions on disk have simple magnetic configuration and did not show any significant flaring activity. The solar flaring activity is likely to be at low levels over the coming days with C-class flares expected and M-class flares possible.

Krooniaine massiline väljavool

A Coronal Mass Ejection (CME), was detected at 23:24 UTC on February 19, in LASCO C2 data. The CME is associated with an eruption seen in SDO/AIA 193 at 22:58 UTC on February 19 associated with NOAA AR 3583. Further analysis is ongoing.

Päikesetuul

Slow solar wind conditions were recorded over the past 24 hours. The solar wind speed as measured by ACE, fluctuated between 280 km/s and 357 km/s. The interplanetary magnetic field fluctuated between 2 nT and 8 nT, with the Bz reaching a minimum value of -7 nT. The phi-angle was in the positive sector (directed away the Sun) with periods on the negative sector. In the next 24-hours slow solar wind conditions are expected.

Geomagnetism

The geomagnetic conditions over the past 24 hours were globally and locally quiet (Kp 2 and K Bel 2). Geomagnetic conditions are expected to be at quiet levels over the next 24 hours.

Prootoni voo tasemed

Over the past 24 hours the greater than 10 MeV GOES proton flux continued to decrease and, although still slightly elevated, remained below the 10 pfu threshold. The proton flux is expected to continue to decrease over the next 24 hours.

Elektronivoog geostatsionaarsel orbiidil

The greater than 2 MeV GOES 16 electron flux was below the 1000 pfu threshold and is expected to remain so in the upcoming days. The 24h electron fluence was at nominal level and is expected to remain so in the next days.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 049, põhineb 17 jaamadel.

Päikese indeksid 19 Feb 2024

Catania Wolfi number///
10cm päikesevoog152
AK Chambon La Forêt006
AK Wingst002
Hinnanguline Ap002
Hinnanguline rahvusvaheline päikeselaikude arv075 - Põhineb 17 jaamal

Märkimisväärsete sündmuste kokkuvõte

PäevAlgusMaksLõppLokatsioonTugevusOP10cmCatania/NOAARaadiosignaalipursete tüübid
Puuduvad

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

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