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Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2025 Jun 27 1240 UTC

Prognoza SIDC

Rozbłyski słoneczne

C-class flares expected, (probability >=50%)

Geomagnetyzm

Minor storm expected (A>=30 or K=5)

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
27 Jun 2025	118	019
28 Jun 2025	117	024
29 Jun 2025	116	012

Aktywne obszary słoneczne i rozbłyski

Solar flaring activity was low over the past 24 hours, with only C-class flares identified. The largest flare was a C1.9 flare (SIDC Flare 4765) peaking on June 27 at 03:05 UTC, which was produced by SIDC Sunspot Group 533 (NOAA Active Region 4122). During the flare, the source region (AR 4122) of the flare had beta configuration of its photospheric magnetic field. A total of 5 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 530 (NOAA Active Region 4120) is the complex region with its beta-gamma magnetic configurations. The solar flaring activity is expected to be at low to moderate levels over the next 24 hours with C-class flares expected, M-class flares probable, and a small chance of X-class flares.

Koronalny wyrzut masy

No Earth-directed coronal mass ejections (CME) were detected in the available coronagraph observations during last 24 hours.

Wiatr słoneczny

Earth is still inside a fast solar wind stream, with the continuous arrival of high speed streams (HSSs) from the large SIDC Coronal Hole 116 (negative polarity) which started to cross the central meridian on Jun 21. The solar wind speed ranged from 595 km/s to 810 km/s. The interplanetary magnetic field ranged between 3 nT and 11 nT, and the North- South component (Bz) ranged betweeen -9 nT and 9 nT. In the next 24 hours, enhanced solar wind conditions are expected to continue with the further arrival of HSSs from the same coronal hole.

Geomagnetyzm

Geomagnetic conditions were globally at unsettled to minor storm conditions (NOAA Kp 3 to 5), and locally at quiet to active conditions (K_BEL 2 to 4) during the past 24 hours. The disturbed geomagnetic conditions was due to the further arrival of high speed streams (HSSs) from the large SIDC Coronal Hole 116 (negative polarity) which started to cross the central meridian on Jun 21. In the next 24 hours, unsettled to minor storm conditions (K 3 to 5) are possible with the continuous arrival of HSSs from the same coronal hole.

Poziomy przepływu protonów

The greater than 10 MeV GOES proton flux was below the threshold level over the past 24 hours and it is expected to remain so for the next 24 hours.

Strumienie elektronów na orbicie geostacjonarnej

The greater than 2 MeV electron flux, as measured by GOES-19 and GOES-18 satellites, remained below the 1000 pfu threshold level almost all the time, except for brief instance around 11:30 UTC and 07:30 UTC on Jun 27, respectively, during which they exceeded the threshold level. In the next 24 hours, the electron flux may briefly exceed the threshold level. The 24h electron fluence is presently at normal level, and it is expected to remain so in the next 24 hours.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 119, na podstawie 15 stacji.

Indeksy solarne na 26 Jun 2025

Liczba Wolfa z Katanii	100
Fale radiowe 10,7 cm	117
AK Chambon La Forêt	037
AK Wingst	031
Szacunkowa Ap	031
Szacowana międzynarodowa liczba plam słonecznych	101 - Na podstawie stacji 21

Podsumowanie wydarzeń godnych uwagi

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

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