Vaata teisipäev, 18 august 2020 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2020 Aug 18 1237 UTC

SIDC ennustus

Kehtib alates 1230 UTC, 18 Aug 2020 kuni 20 Aug 2020
Päikesepursked ehk loited

Quiet conditions (<50% probability of C-class flares)

Geomagnetism

Quiet (A<20 and K<4)

Päikese prootonid

Quiet

10 cm voolAp
18 Aug 2020071003
19 Aug 2020071008
20 Aug 2020071014

Bülletään

The solar activity was low over the past 24 hours. The N0AA-AR 2771 is still on the disk. The X-ray flux was at A-class level and the solar activity is expected to remain low.

The Coronal Mass Ejection (CME) that took place on Aug 16th 18:00UT has a small chance of a glancing blow from late Aug 19th.

The greater than 10 MeV proton flux was at background levels over the past 24 hours. It is expected to stay at background levels for the next 24 hours. The greater than 2 MeV electron flux fluctuated between nominal and moderate levels over the past 24 hours. It is expected to remain nominal to moderate levels over the next 24 hours.

The solar wind speed near Earth varied between 280 and 340km/s (DSCOVR). The polarity of the Interplanetary Magnetic Field (IMF) was predominantly oriented away the Sun (phi angle in the positive sector). Bz fluctuated between -6 and +5 nT. The magnitude of the magnetic field varied between 1 and 7 nT. A negative coronal hole crossed the central meridian on August 17th. An enhancement could be expected on Aug 20th, possibly combined with any effects from the CME. For the first part of the next 24 hours, the solar wind speed is expected to remain low, while by the end of Aug 19th to be enhanced as a response to the influence of the CME.

The geomagnetic conditions were quiet. The values registered for the past 24 hours were 0-2 for K Dourbes and NOAA Kp. Quiet geomagnetic conditions are expected for the next 24 hours. The solar wind speed near Earth varied between 280 and 340km/s (DSCOVR). The polarity of the Interplanetary Magnetic Field (IMF) was predominantly oriented away the Sun (phi angle in the positive sector). Bz fluctuated between -6 and +5 nT. The magnitude of the magnetic field varied between 1 and 7 nT. A negative Coronal hole crossed the central meridian on August 17th. An enhancement could be expected on Aug 20th, possibly combined with any effects from the CME. For the next 24 hours the solar wind speed is expected to remain low for the beginnig of that time period, while by the end of Aug 19th to be enhanced as a response to the influence of the CME.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 012, põhineb 21 jaamadel.

Päikese indeksid 17 Aug 2020

Catania Wolfi number///
10cm päikesevoog071
AK Chambon La Forêt008
AK Wingst004
Hinnanguline Ap003
Hinnanguline rahvusvaheline päikeselaikude arv000 - Põhineb 30 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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