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Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2017 Sep 24 1230 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
24 Sep 2017	084	009
25 Sep 2017	087	016
26 Sep 2017	090	007

Skrót wiadomości

Over the past 24 hours the solar activity was very low. Only small B-class flares and one non-Earth directed slow-speed CME were recorded. Catania sunspot groups 56 (NOAA active regions 2681) has increased its magnetic complexity (from Alpha to Beta class), but has not shown any flaring activity. The returning region NOAA active region 2682 (previously, Catania sunspot group 46, NOAA active region 2673) is now on the visible disc and is the source of the slow-speed CME and B-class flaring activity. Its magnetic complexity is difficult to estimate due to the projection effect, however, it seems to have drastically decay from the previous solar rotation. We expect the solar activity to increase due to the return of this region with C-class flares.

No Earth directed CMEs have been observed and the solar protons remained at background level over the past 24 hours. The Earth remained inside a slow solar wind flow. The speed has further decreased from about 400 to 330 Km/s. The interplanetary magnetic field magnitude remained below 6 nT and the Bz component fluctuated between -5 and 5 nT. The associated fast solar wind to the small equatorial coronal hole that has crossed the central meridian on Sept 20 has not arrived yet and is expected to arrive at Earth today. A new larger coronal hole with positive polarity is currently facing Earth. This coronal hole is elongated from the north solar pole to the solar Equator and its high speed stream is expected to arrive at Earth in about 3 days from now (on Sept 27).

Geomagnetic conditions were quiet with Kp (NOAA) and local K (Dourbes) indexes ranging between 1-2. The geomagnetic conditions are expected to become more active with the arrival of the high speed stream from the coronal hole that has crossed the central meridian on Sept 20. As this coronal hole was relatively small, no strong or sever magnetic storm is expected.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 023, na podstawie 18 stacji.

Indeksy solarne na 23 Sep 2017

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	081
AK Chambon La Forêt	009
AK Wingst	007
Szacunkowa Ap	005
Szacowana międzynarodowa liczba plam słonecznych	013 - Na podstawie stacji 27

Podsumowanie wydarzeń godnych uwagi

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

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