Przeglądasz Archiwum z niedziela, 31 października 2021

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2021 Oct 31 1242 UTC

Prognoza SIDC

Rozbłyski słoneczne

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

Geomagnetyzm

Quiet (A<20 and K<4)

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
31 Oct 2021	110	007
01 Nov 2021	108	001
02 Nov 2021	103	001

Skrót wiadomości

Solar flaring activity was low during the last 24 hours, with seven C-class flares detected from two Active Regions (ARs). More specifically, NOAA AR 2887 produced two C-class flares and NOAA AR 2891 produced the remaining five. NOAA AR 2887 has now lost a significant portion of its magnetic complexity and is not expected to produce any X-class flares. There is a reduced but significant chance for an isolated M-class flare and the C-class flare activity is expected from this AR for the next 24 hours. NOAA AR 2891 is expected to continue its C-class flare activity, with a small chance of an M-class flare, in the next 24 hours.

No Earth-directed Coronal Mass Ejections (CMEs) can be seen in the available corona images.

The greater than 10 MeV proton flux as measured by GOES-16 dropped below nominal levels during the last 24 hours. It is expected to remain below this level for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain below this threshold during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.

The solar wind (SW) conditions were affected by an Interplanetary Coronal Mass Ejection (ICME) that arrived around 30 Oct 17:00 UT, as predicted. The SW speed increased from a background value of 310 km/s to 460 km/s during the last 24 hours. The total magnetic field varied between 2 and 13 nT, while the Bz varied between -11 and +8 nT in the last 24 hours. The interplanetary magnetic field phi angle was predominantly in the positive sector (directed away from the Sun) during the last 24 hours. The electron temperature increased from a background level of approximately 20000 K to 100000 K during the last 24 hours. Since the ICME arrival had a relatively small impact, geomagnetic conditions are expected to gradually return to a slow wind regime during the next 24 hours.

Geomagnetic conditions were globally and locally quiet to moderate (Kp and K Dourbes indeces 1-4). The moderate levels were the result of the expected ICME that arrived around 30 Oct 17:00 UT. However the impact of its arrival is relatively small and short-lived, hence the geomagnetic conditions are expected to be quiet for the next 24 hours.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 063, na podstawie 15 stacji.

Indeksy solarne na 30 Oct 2021

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	107
AK Chambon La Forêt	017
AK Wingst	010
Szacunkowa Ap	010
Szacowana międzynarodowa liczba plam słonecznych	073 - Na podstawie stacji 17

Podsumowanie wydarzeń godnych uwagi

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

Wszystkie czasy w UTC

<< Idź do codziennego przeglądu