Przeglądasz Archiwum z czwartek, 15 lutego 2018

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2018 Feb 15 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
15 Feb 2018	075	015
16 Feb 2018	074	012
17 Feb 2018	073	012

Skrót wiadomości

Over the past 24 hours solar activity has been low. No significant flares have been recorded. Active Region (AR) 2699 (Mcintosh class:Dso; Mag. type:Beta) has been most active, showing considerable flux emergence and cancellation. The greater than 10MeV proton flux remained at background levels over the past 24 hours. No Earth directed Coronal Mass Ejections (CMEs) have been detected. Over the next 24 hours there is a reasonable probability that flaring activity will reach C-class levels with a small probability of M-class flares. The solar wind speed fluctuated around 310 km/s over the past 24 hours, but jumped to 350 km /s this morning with the arrival of a shock front. The total magnetic field strength has remained around 3 nT, but began fluctuating between 3 and 9 nT in the last few hours. The Bz component has fluctuated between -3 and +3 nT. Geomagnetic conditions ranged between Kp index 0-2 (NOAA) and local K index 0-2 (Dourbes) over the past 24 hours. The above mentioned shock front arrived at 07:55 UT this morning. The sudden increase in the solar wind speed (from about 310 to 350 km/s) was observed simultaneously with an increase in the density, temperature and the interplanetary magnetic field magnitude (from about 2 nT to 7 nT). Since the solar wind speed was, and is still rather low, and the Bz component of the interplanetary magnetic field was mostly positive, the shock arrival did not induce disturbed geomagnetic conditions. The shock is probably related to the CME produced at 01:25 UT on 12-Feb-2018, which was anticipated to arrive at approximately 12:00 UT today. A large coronal hole that passed the central meridian a couple of days ago may also be the cause, however the associated High Speed Stream (HSS) is expected to arrive later today / tomorrow. Enhanced solar wind conditions from the coronal hole and CME arrival are expected to cause geomagnetic conditions to be unsettled.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 016, na podstawie 10 stacji.

Indeksy solarne na 14 Feb 2018

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	075
AK Chambon La Forêt	007
AK Wingst	003
Szacunkowa Ap	003
Szacowana międzynarodowa liczba plam słonecznych	023 - Na podstawie stacji 22

Podsumowanie wydarzeń godnych uwagi

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

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