Vaata laupäev, 8 aprill 2017 arhiivi

SIDC igapäevane bülletään päikese ja geomagnetilise aktiivsuse kohta

Välja antud: 2017 Apr 08 1230 UTC

SIDC ennustus

Kehtib alates 1230 UTC, 08 Apr 2017 kuni 10 Apr 2017
Päikesepursked ehk loited

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

Geomagnetism

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

Päikese prootonid

Quiet

10 cm voolAp
08 Apr 2017072018
09 Apr 2017072016
10 Apr 2017070013

Bülletään

Solar activity was at low levels during the period. Three C-class flares were recorded, the strongest being a C4.3 event at 19:49UT. These flares originated from NOAA 2645's trailing portion, which has rotated over the west limb. The Sun is currently spotless. A small active region, responsible for a B3 flare at 01:48UT, is about to rotate over the east limb. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10MeV proton flux was at nominal levels.

An isolated C-class flare remains possible.

Around 17UT, solar wind speed started a gradual increase from its nominal 420 km/s to end the period at 570 km/s and still climbing. Bz fluctuated between -8 and +6 nT. The interplanetary magnetic field was initially directed towards the Sun, but became variable after 17UT to end the period in a steady towards direction. The particle stream from a narrow extension from the positive polar coronal hole may affect the earth environment on 9 or 10 April.

The geomagnetic field was at quiet to unsettled levels, with active episodes (Kp=4) during 21UT-03UT and 06-09UT. Dourbes geomagnetic data were missing for most of the period, but Wingst and Niemegk showed an active episode around midnight too. The geomagnetic field is expected to be at quiet to active levels, in response to particle streams from various coronal holes.

Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 000, põhineb 23 jaamadel.

Päikese indeksid 07 Apr 2017

Catania Wolfi number034
10cm päikesevoog074
AK Chambon La Forêt017
AK Wingst012
Hinnanguline Ap012
Hinnanguline rahvusvaheline päikeselaikude arv023 - 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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