Vaata kolmapäev, 23 august 2023 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2023 Aug 23 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
23 Aug 2023151007
24 Aug 2023153007
25 Aug 2023155007

Päikese aktiivsed piirkonnad ja pursked

There are eight active regions visible on the disk, a new region rotated over the east limb (NOAA AR 3415). They all have simple alpha or beta magnetic field configuration. An M1.1 flare occurred on 22 August, with peak at 23:04 UTC, from NOAA AR 3405. C-class flares are expected and M-class flares are possible in the next 24 hours.

Krooniaine massiline väljavool

A wide CME (angular width around 80 degrees) erupted to the west, first seen at 19:00 UTC on 22 August by LASCO-C2. The source region of this CME is slightly backsided and thus the CME will not arrive to the Earth. About 1 hour later, a faint CME could be seen erupting towards the southeast, related to dimmings seen on EUV around NOAA ARs 3405 and 3411 (this activity is also related to the M1.1 flare from NOAA AR 3405). Due to the location of the dimmings (close to disk center), a possible arrival to the Earth of this faint CME cannot be discarded (on 26 August). Later on, one more faint CME erupted from NOAA AR 3404, in the vicinity of the previous eruption and first seen at 02:00 UTC by LASCO-C2. This last CME will most likely not affect Earth (although more data will be investigated as it becomes available).

Päikesetuul

The Earth is inside a slow solar wind stream, with speed around 430 km/s and an interplanetary magnetic field around 5 nT. The interplanetary magnetic field orientation was predominantly in the negative sector (field directed towards the Sun). Similar conditions can be expected in the next 24 hours.

Geomagnetism

During the last 24 hours the geomagnetic conditions were quiet (NOAA KP 1-2, K Bel 1-2). Similar conditions can be expected for the next 24 hours.

Prootoni voo tasemed

Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next 24 hours.

Elektronivoog geostatsionaarsel orbiidil

The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain so in the next 24 hours. The 24 hour electron fluence was at normal levels and is expected to remain so.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 105, põhineb 23 jaamadel.

Päikese indeksid 22 Aug 2023

Catania Wolfi number127
10cm päikesevoog151
AK Chambon La Forêt010
AK Wingst008
Hinnanguline Ap008
Hinnanguline rahvusvaheline päikeselaikude arv119 - Põhineb 28 jaamal

Märkimisväärsete sündmuste kokkuvõte

PäevAlgusMaksLõppLokatsioonTugevusOP10cmCatania/NOAARaadiosignaalipursete tüübid
22223523042338N11W29M1.1SF27/3405CTM/2VI/2

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

Kõik ajad UTC-s

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