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Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2025 Apr 18 1231 UTC

Prognoza SIDC

Rozbłyski słoneczne

M-class flares expected (probability >=50%)

Geomagnetyzm

Active conditions expected (A>=20 or K=4)

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
18 Apr 2025	153	011
19 Apr 2025	155	014
20 Apr 2025	157	017

Aktywne obszary słoneczne i rozbłyski

Solar flaring activity over the last 24 hours has been low, with few C-class flares only. The strongest flare was a C4.6 flare (SIDC Flare 4149) peaking at 14:22 UTC on April 17, associated with SIDC Sunspot Group 474 (NOAA Active Region 4064, magnetic type beta). There are currently seven numbered active regions on the solar disk. The most complex one is SIDC Sunspot Group 450 (NOAA Active Region 4060, magnetic type beta-delta). A new, currently unnumbered active region (SIDC Sunspot Group 478, magnetic type beta) has rotated on disk from the east limb. The solar flaring activity is expected to be low to moderate over the next 24 hours, with C-class flares expected and M-class flares probable.

Koronalny wyrzut masy

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

Dziury koronalne

The southern, mid-latitude, positive polarity coronal hole (SIDC Coronal Hole 104) continues to cross the central meridian since April 17. An associated high-speed stream may arrive at Earth starting from the UTC evening of April 19.

Wiatr słoneczny

The solar wind conditions (ACE and DSCOVR) were enhanced over the last 24 hours, under the waning effect of the interplanetary Coronal Mass Ejection (ICME) arrivals, associated with the CMEs that lifted on April 12 and April 13, and a possible high-speed stream arrival from SIDC Coronal Hole 105. The solar wind speed was mostly around 450 km/s. The interplanetary magnetic field decreased from 13 nT to 7 nT. The Bz component was mostly positive, decreasing from 11 nT to 2 nT, with a period of negative values (reaching a minimum of -10 nT) between 00:30 UTC and 05:30 UTC on April 18. The interplanetary magnetic field angle was predominantly in the negative sector. Currently, the solar wind speed is around 450 km/s, the interplanetary magnetic field around 6 nT and the Bz component between 1 nT and 5 nT. Enhanced solar wind conditions may be expected over the next 24 hours.

Geomagnetyzm

Geomagnetic conditions globally reached active levels (NOAA Kp 4) between 06:00 UTC and 09:00 UTC on April 18. Geomagnetic conditions locally were mostly at unsettled levels (K BEL 3) until 06:00 UTC on April 18 and have since decreased to quiet levels (K BEL 2). Mostly unsettled to active levels (NOAA Kp 3 to 4, K BEL 3 to 4) are expected globally and locally over the next 24 hours.

Poziomy przepływu protonów

The greater than 10 MeV proton flux was below the threshold level over the past 24 hours. It is expected to remain below the threshold level over the next 24 hours.

Strumienie elektronów na orbicie geostacjonarnej

The greater than 2 MeV electron flux measured by GOES 18 and GOES 19 was below the threshold over the past 24 hours. The greater than 2 MeV electron flux is expected to remain below the threshold over the next 24 hours. The 24-hour electron fluence is presently at normal levels and is expected to remain so over the next 24 hours.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 114, na podstawie 11 stacji.

Indeksy solarne na 17 Apr 2025

Liczba Wolfa z Katanii	///
Fale radiowe 10,7 cm	151
AK Chambon La Forêt	018
AK Wingst	011
Szacunkowa Ap	012
Szacowana międzynarodowa liczba plam słonecznych	099 - Na podstawie stacji 16

Podsumowanie wydarzeń godnych uwagi

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

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