Vaata esmaspäev, 18 november 2024 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2024 Nov 18 1246 UTC

SIDC ennustus

Päikesepursked ehk loited

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

Geomagnetism

Quiet (A<20 and K<4)

Päikese prootonid

Quiet

10 cm voolAp
18 Nov 2024156015
19 Nov 2024160011
20 Nov 2024170010

Päikese aktiivsed piirkonnad ja pursked

Solar flaring activity was high over the past 24 hours, with 5 M-class flares. The largest flare was an M2.5 flare peaking on November 18 at 10:58 UTC from an as yet unnumbered region rotating over the south-east limb. SIDC Sunspot Group 288 (NOAA Active Region 3889) the other largest region on disk also produced C-class flaring activity but is now approaching the east limb. The solar flaring activity is expected to be moderate over the next 24 hours, with M-class flares likely and a small chance for X-class flares.

Krooniaine massiline väljavool

No Earth-directed coronal mass ejections (CMEs) have been detected in the available coronagraph imagery over the past 24 hours.

Krooniauk

SIDC Coronal Hole 79 (mid-latitude coronal hole with a negative polarity) has begun to cross the central meridian on November 18.

Päikesetuul

Over the past 24 hours the solar wind conditions reflected a slow solar wind regime. The interplanetary magnetic field continued to be slightly elevated, ranging between 5 and 9nT, with a minimum Bz of -7 nT. The solar wind speed ranged between 310 and 380 km/s. The interplanetary magnetic field phi angle remained predominantly in the positive sector (directed towards the Sun). The solar wind speed is expected to become slightly elevated over the next 24 hours due to the possible high-speed stream arrival associated with SIDC Coronal Hole 78, although this is low confidence.

Geomagnetism

The geomagnetic conditions over the past 24 hours were quiet to unsettled. Quiet to unsettled geomagnetic conditions are expected for the next 24 hours with isolated active conditions possible due to any high- speed stream influence.

Prootoni voo tasemed

Over the past 24 hours the greater than 10 MeV GOES proton flux was below the 10 pfu threshold. The greater than 10 MeV GOES proton flux is expected to continue to be below this threshold over the 24 hours.

Elektronivoog geostatsionaarsel orbiidil

The greater than 2 MeV electron flux as measured by GOES 18 crossed the 1000 pfu threshold briefly and is expected to again be at or near this threshold over the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so in the next 24 hours.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 110, põhineb 12 jaamadel.

Päikese indeksid 17 Nov 2024

Catania Wolfi number///
10cm päikesevoog146
AK Chambon La Forêt011
AK Wingst006
Hinnanguline Ap006
Hinnanguline rahvusvaheline päikeselaikude arv085 - Põhineb 14 jaamal

Märkimisväärsete sündmuste kokkuvõte

PäevAlgusMaksLõppLokatsioonTugevusOP10cmCatania/NOAARaadiosignaalipursete tüübid
18051305220527----M1.0--/3901
18072507320736S07E76M1.7SF--/3901
18075407570801S07E76M1.21--/3901III/2
18104110581102S07E76M2.5SF--/3901
18110611121119----M1.6--/----III/2

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

Kõik ajad UTC-s

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