Datum verslag: 2026 Jun 20 1231 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 20 Jun 2026 | 111 | 006 |
| 21 Jun 2026 | 113 | 007 |
| 22 Jun 2026 | 115 | 007 |
A total of 4 numbered sunspot groups were identified on the disk over the past 24 hours. An M1.3 flare (the largest of the period) was observed peaking on June 20 at 01:51 UTC, which was produced by SIDC Sunspot Group 897 (NOAA Active Region 4472) that rotated into view from the east limb. More M-class flares are possible in the coming 24 hours.
A wide Coronal Mass Ejection (CME) with an angular width of approximately 90 degrees was detected by LASCO C2 at 02:12 UTC on 20 June. Associated with an M1.3 solar flare, this CME originated near the east limb and is directed eastward; no Earth arrival is expected. Shortly after, at 03:12 UTC, a second CME emerged toward the northeast. While spatial and temporal proximity causes these CMEs to appear merged in coronagraph imagery, they are distinct events. The second CME originated on the farside of the Sun and will not impact Earth.
In the last 24 hours we saw a slight increase in solar wind speed (up to 450 km/s) and magnetic field (11 nT) related to the expected mild fast stream from SIDC Coronal Hole 169. The Earth is currently inside slow solar wind, the solar wind speed is around 400 km/s and the interplanetary magnetic field is at 7nT. Similar conditions can be expected for the next 24 hours.
Geomagnetic conditions were quiet to unsettled both at planetary and local levels (Kp and K_Bel up to 3). Similar conditions can be expected for the next 24 hours.
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, as measured by GOES-18 and GOES-19 was below the 1000 pfu alert threshold in the past 24 hours. The flux is expected to remain low over the next 24 hours. The 24-hour electron fluence was at normal levels over the past 24 hours and is expected to remain at these levels over the next 24 hours.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 089, gebaseerd op 20 stations.
| Wolfgetal Catania | 053 |
| 10cm zonneflux | 111 |
| AK Chambon La Forêt | 013 |
| AK Wingst | 008 |
| Geschatte Ap | 009 |
| Geschat internationaal zonnevlekkengetal | 066 - Gebaseerd op 29 stations |
| Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
|---|---|---|---|---|---|---|---|---|---|
| 20 | 0126 | 0151 | 0204 | ---- | M1.3 | 54/4472 |
Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive
Alle tijden in UTC
<< Keer terug naar de dagelijkse overview pagina
Veel mensen komen naar Poollicht.be om de zonneactiviteit te volgen of om het poollicht te zien, maar met meer bezoekers komen er hogere kosten bij om de servers online te houden. Als je Poollicht.be leuk vindt en het project wilt steunen, kun je kiezen voor een abonnement op een advertentievrije website of een donatie overwegen. Met jouw hulp kunnen we Poollicht. be online houden!
| Laatste X-klasse uitbarsting | 03/06/2026 | X1.0 |
| Laatste M-klasse uitbarsting | 21/06/2026 | M6.9 |
| Laatste geomagnetische storm | 11/06/2026 | 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 | 97.5 -3.9 |
| Afgelopen 30 dagen | 107.9 +10.3 |