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Tägliches Bulletin zur solaren und geomagnetischen Aktivität des SIDC

Ausgestellt: 2025 Sep 09 1239 UTC

Vorhersage des SIDC

Sonneneruptionen

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

Geomagnetismus

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

Sonnenprotonen

Quiet

	10cm Fluss	Ap
09 Sep 2025	123	013
10 Sep 2025	121	013
11 Sep 2025	120	007

Solaraktive Regionen und Flares

Solar flaring activity was low over the past 24 hours, with only C-class flares identified. The largest flare was a C1.5 flare (SIDC Flare 5464) peaking on September 09 at 03:23 UTC, which was produced by SIDC Sunspot Group 624 (NOAA Active Region 4207). During the flare, the source region (AR 4207) of the flare had beta configuration of its photospheric magnetic field. A total of 6 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Groups 624, 628, 630, and 631 (NOAA Active Regions 4207, 4210, 4212, and 4213) are the complex regions with its beta magnetic configurations. Solar flaring activity is expected to be at low to moderate levels over the next 24 hours, with C-class flares expected and a small chance for M-class flares.

Koronaler Massenauswurf

A narrow coronal mass ejection (CME) was observed in SOHO/LASCO-C2 images on NW limb at 03:48 UTC on Sep 09 (about 40 deg). It was associated with C1.5 flare (peak: 03:23 UTC, N28 W51) from the SIDC sunspot group 624 (NOAA AR 4207), and it is not expected to arrive at Earth. No other Earth-directed CMEs were detected in the available coronagraph observations during last 24 hour.

Koronale Löcher

Recurrent SIDC Coronal Hole 123 (positive polarity, elongated coronal hole in the southern hemisphere) has crossed the central meridian, and the high speed streams originating from this coronal hole are expected to impact the Earth until Sep 11.

Sonnenwind

Over the past 24 hours, the solar wind parameters remained under the influence of high speed streams (HSSs) from the SIDC Coronal Hole 123 (positive polarity, elongated coronal hole in the southern hemisphere) which crossed the central meridian during Sep 02-09. The solar wind speed ranged from 410 km/s to 640 km/s. The North-South component (Bz) ranged between -5 and 5 nT. The interplanetary magnetic field ranged between 0 nT to 9 nT. In the next 24 hours, enhanced solar wind conditions are expected to continue possibly with the further arrival of HSSs from the same coronal hole.

Geomagnetismus

Geomagnetic conditions were at quiet to unsettled conditions (NOAA Kp 2 to 3), globally and locally during the past 24 hours. We expect quiet to active conditions (K 1 to 4) in the next 24 hours with the further arrival of high speed streams from the SIDC Coronal Hole 123 (positive polarity) which crossed the central meridian during Sep 02-09.

Protonenflusswerte

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.

Elektronenflüsse im geostationären Orbit

Over the past 24 hours, the greater than 2 MeV electron flux, as measured by GOES-18 satellite, remained below the 1000 pfu threshold level almost all the time, except for brief instance around 19:15 UTC and 23:00 UTC on Sep 08 during which it exceeded the threshold level. It was in response to the high solar wind speed associated with the SIDC Coronal Hole 123 (positive polarity) which crossed the central meridian during Sep 02-09. The greater than 2 MeV electron flux, as measured by GOES-19 satellite, remained below 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.

Die heute international geschätzte Sonnenfleckenanzahl (ISN): 103, basierend auf 12 Stationen.

Solarindizes für den 08 Sep 2025

Wolf-Zahl Catania	///
10cm Solarflux	124
AK Chambon La Forêt	017
AK Wingst	014
Geschätzer Ap-Wert	015
Geschätzte internationale Sonnenfleckenzahl	118 - Basierend auf 20 Stationen

Zusammenfassung auffälliger Ereignisse

Zur Verfügung gestellt vom Solar Influences Data Analysis Center© - SIDC - Verarbeitet von SpaceWeatherLive

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