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Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2017 Jul 18 1241 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
18 Jul 2017	084	015
19 Jul 2017	083	017
20 Jul 2017	083	007

Skrót wiadomości

NOAA region 2665 (Catania group 36) produced several C flares and is now located at the West limb. The largest was a C2.0 flare peaking at 00:40UT. As the region is disappearing behind the limb we still anticipate some related C flaring and a chance for an M flare but by the end of the period the region should have passed well around the limb. In SoHO/LASCO C2 a Westbound CME was visible from around 17:00UT onwards. It originated from NOAA region 2665 and was associated to along duration C1.2 flare. The CME had a limited angular extent and it is judged not to be Earth effective. Proton flux levels are at background values and expected to remain so.

Solar wind conditions showed the passage of the wake of the July 14 CME. Total magnetic field remained near 10nT for most of the period before dropping to nominal levels under 4nT around 9:00UT. Solar wind speed was mostly around 520 km/s before increasing to over 600 km/s around 9:00UT with values reaching over 650km/s. This thus seems to mark a transition into a fast solar wind regime around 9:00UT which is possibly due to the negative polarity coronal hole that passed the central meridian on July 14 in the southern hemisphere. Over the next 24-48 hours solar wind is expected to slowly recover towards nominal solar wind conditions. Geomagnetic conditions were mostly quiet to active (local K Dourbes 2-4) while the planetary NOAA Kp reached one isolated episode of moderate storm condition in the wake of the CME passage. With current high solar wind speed but nominal magnetic field values unsettled conditions are expected with isolated active periods possible. As Solar wind speed decreases quiet to unsettled conditions are expected later on.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 000, na podstawie 24 stacji.

Indeksy solarne na 17 Jul 2017

Liczba Wolfa z Katanii	025
Fale radiowe 10,7 cm	086
AK Chambon La Forêt	024
AK Wingst	024
Szacunkowa Ap	026
Szacowana międzynarodowa liczba plam słonecznych	021 - Na podstawie stacji 33

Podsumowanie wydarzeń godnych uwagi

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

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