Vaata reede, 18 august 2023 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2023 Aug 18 1241 UTC

SIDC ennustus

Päikesepursked ehk loited

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

Geomagnetism

Active conditions expected (A>=20 or K=4)

Päikese prootonid

Quiet

10 cm voolAp
18 Aug 2023153013
19 Aug 2023151014
20 Aug 2023148008

Päikese aktiivsed piirkonnad ja pursked

The solar flaring activity was at low levels. The largest flare was a C5.1 flare peaking at 12:40 UTC on August 17, this originated near the west limb associated with NOAA AR3397, which has now rotated over the limb. NOAA AR 3403 decayed over the period and was quiet. NOAA AR3405 also produced C-class flares and has been split into two regions including the small new region NOAA AR3411. NOAA AR3407 and AR3410 were stable and quiet. NOAA ARs 3406, 3408 both decayed into plage region. NOAA AR3409, which began to emerge yesterday has continued to grow and produced low level C-class flares. The solar flaring activity is expected to be at low levels over the next 24 hours with C-class flares likely and a low chance for isolated M-class flares.

Krooniaine massiline väljavool

There were no Earth-directed Coronal Mass Ejections (CMEs) detected in the available coronagraph observations.

Päikesetuul

The solar wind parameters reflected a weak negative polarity high speed stream arrival. The interplanetary magnetic field was slightly enhanced, with a significant increase around 02:00 UTC on August 18, when it jumped from 9 and 14 nT. Bz had a minimum value of -11nT. The solar wind speed increased gradually from 02:00 UTC, from 300km/s to values near 500 km/s. The interplanetary magnetic field orientation switched to the negative sector (field directed towards the Sun) from 19:00 UTC on August 17. The solar wind parameters are expected to remain enhanced on August 18 and 19, while the Earth remains under the influence for the high-speed stream.

Geomagnetism

During last 24 hours the geomagnetic conditions were at quiet to unsettled levels (NOAA KP 1-3 and K-Bel 1-3). Geomagnetic conditions are expected to be at unsettled levels, with active periods possible on August 18 and 19, due to the ongoing high speed stream influence.

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 days.

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 below this threshold over the next days. The 24 hour electron fluence was at nominal levels. The electron fluence is expected to be at nominal levels for the next days.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 125, põhineb 14 jaamadel.

Päikese indeksid 17 Aug 2023

Catania Wolfi number///
10cm päikesevoog152
AK Chambon La Forêt011
AK Wingst010
Hinnanguline Ap009
Hinnanguline rahvusvaheline päikeselaikude arv149 - Põhineb 24 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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