Vaata kolmapäev, 14 märts 2018 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2018 Mar 14 1230 UTC

SIDC ennustus

Päikesepursked ehk loited

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

Geomagnetism

Quiet (A<20 and K<4)

Päikese prootonid

Quiet

	10 cm vool	Ap
14 Mar 2018	069	013
15 Mar 2018	070	007
16 Mar 2018	071	003

Bülletään

Over the past 24 hours solar activity has been low. No significant flares have been recorded. No Active Regions (AR) are present on the disk, however a small bipolar region has emerged in the western hemisphere N15W60. No Earth directed Coronal Mass Ejections (CMEs) have been detected. The greater than 10MeV proton flux remained at background levels over the past 24 hours. A low latitude coronal hole is currently located in the western hemisphere. Solar activity is expected to remain low over the next 24 hours with a low probability of C-class flares. The solar wind speed has fluctuated between 310 and 375 km/s over the past 24 hours. The total magnetic field strength has fluctuated between 2.0 nT and 6.0 nT. The Bz component has fluctuated around 0 between -3.0 and +3.0 nT. Geomagnetic conditions ranged between Kp index 0-1 (NOAA) over the past 24 hours. A low latitude negative polarity northern polar coronal hole passed the central meridian a couple of days ago but has caused no appreciable increase in solar wind speed, however it may enhance geomagnetic conditions over the next couple of days.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 000, põhineb 25 jaamadel.

Päikese indeksid 13 Mar 2018

Catania Wolfi number	000
10cm päikesevoog	069
AK Chambon La Forêt	006
AK Wingst	003
Hinnanguline Ap	002
Hinnanguline rahvusvaheline päikeselaikude arv	000 - Põhineb 22 jaamal

Märkimisväärsete sündmuste kokkuvõte

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

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