Przeglądasz Archiwum z środa, 3 czerwca 2020

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2020 Jun 03 1236 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
03 Jun 2020	071	005
04 Jun 2020	072	008
05 Jun 2020	073	008

Skrót wiadomości

Solar X-ray flux remained below C level throughout the period. NOAA region 2764 in the northern hemisphere decayed to plage and is inactive. The region turning onto the disk in the South is awaiting analysis and is yet unnumbered, but appears to be relatively inactive presently. The overall probability for C flaring is low.

There were no Earth directed Coronal Mass Ejections (CMEs) observed in coronagraph data.

The greater than 10 MeV proton flux levels were at background values and are expected to continue to be at background level. The greater than 2 MeV electron flux has been nominal over the past days.

There is a low latitude extension of the northern polar coronal hole visible that may influence Solar wind conditions starting around late June 6.

Solar wind conditions were nominal, with Solar wind speed in the 320-360 km/s range. Total magnetic field was around and mostly below 5 nT with a variable Bz component. The magnetic field phi angle was mostly in the negative sector with some excursions into the positive sector. Solar wind conditions are expected to be near nominal over the next days, with later an expected sector boundary crossing and possible enhanced conditions by late June 6.

Geomagnetic conditions were quiet (local K Dourbes 0-2 and NOAA Kp 1-2). Quiet to unsettled geomagnetic conditions are expected in the next days.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 010, na podstawie 21 stacji.

Indeksy solarne na 02 Jun 2020

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	070
AK Chambon La Forêt	008
AK Wingst	008
Szacunkowa Ap	007
Szacowana międzynarodowa liczba plam słonecznych	000 - Na podstawie stacji 37

Podsumowanie wydarzeń godnych uwagi

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

Wszystkie czasy w UTC

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