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Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2021 Sep 02 1231 UTC

Prognoza SIDC

Rozbłyski słoneczne

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

Geomagnetyzm

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

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
02 Sep 2021	085	019
03 Sep 2021	085	011
04 Sep 2021	084	007

Skrót wiadomości

X-ray flux was mostly below C level apart from a single C1.2 flare early in the period from Catania group 32 (NOAA 2860). Catania group 33 (NOAA 2859) decayed to plage while Catania group 32 (NOAA 2860), still the most complex region on disc, seems to simplify as it is rotating towards the West limb. A new bipolar region (currently unnumbered) emerged in the South-Western quadrant. It appears stable and inactive. C-flaring is still rather probable in the next 24 hours.

There were no new Earth directed CMEs observed in available coronagraph data.

The greater than 10 MeV proton flux was at background levels and we expect it will remain so in the next 24 hours. The greater than 2 MeV electron flux reached again above the 1000 pfu threshold during its diurnal maximum both yesterday and today. The 24h electron fluence is at moderate levels and we expect it to be normal to moderate over the next days.

The negative polarity coronal hole in the southern hemisphere that is currently transiting the central meridian is expected to influence Solar wind conditions near Earth on September 5.

Solar wind is in a slow Solar wind regime with no obvious signs of arrival of either the August 26 or the August 28 CME. Solar wind speed was mostly in the 305-345 km/s range. Interplanetary magnetic field was below or around 5nT with an unremarkable Bz component. The orientation of the Interplanetary magnetic field was mostly away from the Sun. There is still the possibility of Solar wind conditions to enhance later today with a later than expected arrival of the August 28 CME. If this arrives, enhanced conditions are expected to last into September 3 and 4. Solar wind enhancements related to the fast wind from the negative polarity coronal hole in the southern hemisphere are only expected from September 5 onwards.

Geomagnetic conditions have been quiet (NOAA Kp 0-1 and local K Dourbes 0-2). Active conditions are possible over the next 24-48 hours with the possible August 28 CME arrival.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 032, na podstawie 18 stacji.

Indeksy solarne na 01 Sep 2021

Liczba Wolfa z Katanii	041
Fale radiowe 10,7 cm	084
AK Chambon La Forêt	007
AK Wingst	004
Szacunkowa Ap	004
Szacowana międzynarodowa liczba plam słonecznych	033 - Na podstawie stacji 22

Podsumowanie wydarzeń godnych uwagi

Dostarczone przez Centrum Analizy Danych Wpływów Słonecznych© - SIDC - Przetworzone przez SpaceWeatherLive

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