Przeglądasz Archiwum z czwartek, 1 października 2020

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2020 Oct 01 1230 UTC

Prognoza SIDC

Rozbłyski słoneczne

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

Geomagnetyzm

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

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
01 Oct 2020	072	010
02 Oct 2020	071	003
03 Oct 2020	071	003

Skrót wiadomości

The solar activity was at very low levels with no significant flares recorded. The solar disk remains spotless and no significant flares are expected over the next 24 hours.

No Earth-directed Coronal Mass Ejections (CMEs) were observed in the available coronagraph imagery.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux was continuously recorded above the 10^3 pfu threshold over the past 24 hours and is currently greater than 10^4 pfu. The electron flux is expected to remain elevated over the next 24 hours.

Over the past 24 hours the solar wind conditions were slightly enhanced under the waning influence of the high-speed stream. The total interplanetary magnetic field, as recorded by ACE and DSCOVR, varied between 1.6 nT and 4.6 nT with a north-south component fluctuating in the range of -4 nT and 4 nT. In the past 24 hours the solar wind speed declined from initially 640 km/s down to 507 km/s. The solar wind conditions are expected to gradually return to background levels over the next 24 hours.

The geomagnetic conditions over the past 24 hours were mostly quiet to unsettled with isolated active periods. The maximum recorded value for Kp and K Dourbes indices is 4. Mostly quiet to unsettled conditions are expected for the next 24 hours with possible isolated active periods.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 000, na podstawie 13 stacji.

Indeksy solarne na 30 Sep 2020

Liczba Wolfa z Katanii	000
Fale radiowe 10,7 cm	073
AK Chambon La Forêt	022
AK Wingst	021
Szacunkowa Ap	020
Szacowana międzynarodowa liczba plam słonecznych	000 - Na podstawie stacji 31

Podsumowanie wydarzeń godnych uwagi

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

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