Przeglądasz Archiwum z niedziela, 28 czerwca 2020

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2020 Jun 28 1241 UTC

Prognoza SIDC

Rozbłyski słoneczne

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

Geomagnetyzm

Quiet (A<20 and K<4)

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
28 Jun 2020	069	005
29 Jun 2020	070	005
30 Jun 2020	070	005

Skrót wiadomości

Solar flaring activity was at very low levels. No significant flares have been recorded. Solar activity is expected to remain at very low levels.

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

The greater than 10 MeV proton flux was at background levels the past 24 hours. It is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux was at nominal levels over the past 24 hours and is expected to stay at nominal levels for the next 24 hours.

The solar wind speed near Earth varied between 340 and 430 km/s (DSCOVR). The polarity of the Interplanetary Magnetic Field (IMF) was predominantly oriented towards the Sun (phi angle in the negative sector). Bz fluctuated between -4 and +7 nT. The magnitude of the magnetic field varied between 3 and 10 nT. The coronal hole crossing central meridian June 27rd seems to have started dissipating. For the next 24 hours the solar wind speed is expected to remain on those levels, with slight possible enhancements, reflecting the influence of the current patchy solar disk.

The geomagnetic conditions were quiet to unsettled with an isolated active period, while the values registered for the past 24 hours were 1-4 for K Dourbes and 1-3 for NOAA Kp. Quiet to unsettled (K Dourbes = 3) geomagnetic conditions are expected for the next 24 hours.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 003, na podstawie 18 stacji.

Indeksy solarne na 27 Jun 2020

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	069
AK Chambon La Forêt	015
AK Wingst	010
Szacunkowa Ap	011
Szacowana międzynarodowa liczba plam słonecznych	003 - Na podstawie stacji 27

Podsumowanie wydarzeń godnych uwagi

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

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