Vaata teisipäev, 5 märts 2024 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2024 Mar 05 1237 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
05 Mar 2024139010
06 Mar 2024139010
07 Mar 2024140007

Päikese aktiivsed piirkonnad ja pursked

The solar flaring activity was low during the last 24 hours with few C-class flares. The strongest reported flare was GOES C2.7 flare which peaked at 11:25 UTC today. During the flare, the source region (AR 3598) of the flare had beta configuration of its photospheric magnetic field. The solar flaring activity is expected to be at low to moderate levels over the next 24 hours with few C-class flares, and a low chance for M-class flares.

Krooniaine massiline väljavool

No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph observations during last 24 hour.

Krooniauk

A small high latitude northern coronal hole (negative polarity) has crossed the central meridian on Mar 05, and it will not possibly impact the Earth. Another very small equatorial (negative polarity) coronal hole is crossing the central meridian on Mar 05. The solar wind from this coronal hole may enhance the solar wind environment near Earth on Mar 08.

Päikesetuul

Solar wind parameters are transitioning from fast to slow solar wind regime. The solar wind speed ranged between 350 km/s and 450 km/s. The North-South component (Bz) ranged between -5 and 10 nT. The interplanetary magnetic field has decreased from 12 nT to 5 nT. Slow solar wind conditions are expected to continue over the next 24 hours.

Geomagnetism

Geomagnetic conditions were globally and locally quiet to unsettled conditions (NOAA Kp and K BEL 1 to 3). Quiet to unsettled conditions are expected in the next 24 hours.

Prootoni voo tasemed

The greater than 10 MeV proton flux was below the threshold level over the past 24 hours and is expected to remain so for the next 24 hours.

Elektronivoog geostatsionaarsel orbiidil

The greater than 2 MeV electron flux, as measured by the GOES-16 satellite, was below the threshold level in the last 24 hours. It is expected that this parameter to remain below the threshold level in the next 24 hours. The 24h electron fluence is presently at normal level and is expected to remain so in the coming 24 hours.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 112, põhineb 08 jaamadel.

Päikese indeksid 04 Mar 2024

Catania Wolfi number134
10cm päikesevoog140
AK Chambon La Forêt014
AK Wingst009
Hinnanguline Ap009
Hinnanguline rahvusvaheline päikeselaikude arv110 - Põhineb 30 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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