Datum verslag: 2026 Jun 25 1231 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 25 Jun 2026 | 141 | 040 |
| 26 Jun 2026 | 140 | 028 |
| 27 Jun 2026 | 138 | 024 |
Solar flaring activity was low over the past 24 hours, with only C-class flares. The largest flare was a C4.3 flare (SIDC Flare 8016) peaking on June 25 at 00:22 UTC, which was produced by SIDC Sunspot Group 902 (NOAA Active Region 4478). A total of 8 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 899 (NOAA Active Region 4475) has the most complex magnetic configuration (Beta-Gamma). SIDC Sunspot Group 899 (NOAA Active Region 4475) and SIDC Sunspot Group 902 (NOAA Active Region 4478) are in charge of the majority of the flaring activity of the past 24 hours. Solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a chance for M-class flares.
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.
The northern mid latitude negative polarity SIDC Coronal Hole 142 just finished crossing central meridian.
The solar wind parameters became slightly disturbed, following the arrival of the high speed stream. The solar wind speed around 700 km/s and an interplanetary magnetic field of 7nT, and BZ reaching a maximum negative value of -9nT. Similar conditions can be expected for the next 24 hours.
Geomagnetic conditions active to minor storm levels globally and unsettled to active at local levels (Kp up to 5, K_Dourbes up to 4). Active to minor storm conditions can be expected for the next 24 hours, under the continued influence of high speed stream.
The greater than 10 MeV proton flux, as measured by GOES-18, was below the 10 pfu threshold level over the past 24 hours and is expected to remain so for the next 24 hours.
The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, and is expected to remain below the threshold during the next 24 hours. The 24h electron fluence was at normal levels and is expected to remain so.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 094, gebaseerd op 22 stations.
| Wolfgetal Catania | 144 |
| 10cm zonneflux | 137 |
| AK Chambon La Forêt | 033 |
| AK Wingst | 020 |
| Geschatte Ap | 020 |
| Geschat internationaal zonnevlekkengetal | 098 - Gebaseerd op 31 stations |
| Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Geen | ||||||||||
Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive
Alle tijden in UTC
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| Laatste X-klasse uitbarsting | 03/06/2026 | X1.0 |
| Laatste M-klasse uitbarsting | 21/06/2026 | M6.9 |
| Laatste geomagnetische storm | 25/06/2026 | Kp5 (G1) |
| Zonnevlekkenloze dagen | |
|---|---|
| Afgelopen 365 dagen | 3 dagen |
| 2026 | 3 dagen (2%) |
| Laatste zonnevlekkenloze dag | 24/02/2026 |
| Maandelijks gemiddeld zonnevlekkengetal | |
|---|---|
| mei 2026 | 101.4 +22.1 |
| juni 2026 | 100.6 -0.8 |
| Afgelopen 30 dagen | 107.3 +10 |