Datum verslag: 2023 Aug 20 1234 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 20 Aug 2023 | 148 | 015 |
| 21 Aug 2023 | 146 | 011 |
| 22 Aug 2023 | 145 | 007 |
The solar flaring activity was at low levels. The largest flare was a C3.7 flare peaking at 06:26 UTC on August 20, associated with NOAA AR3409. NOAA AR3409 has, however, decayed significantly over the period. NOAA AR 3403 also produced low C-class flares. The remaining regions were mostly stable or in decay and were quiet. The solar flaring activity is expected to be at low levels over the next 24 hours with C-class flares likely and a low chance for isolated M-class flares.
There were no Earth-directed Coronal Mass Ejections (CMEs) detected in the available coronagraph observations.
The solar wind parameters showed further enhancement. The interplanetary magnetic field increased from 3 nT to near 10nT. Bz had a minimum value of -6 nT. The solar wind speed increased further from 450km/s to 690 km/s. The interplanetary magnetic field orientation was predominantly in the negative sector (field directed towards the Sun). The solar wind parameters are expected to remain enhanced on August 20 and 21, while the Earth remains under the influence for the high-speed stream, slowly returning to nominal conditions from on August 22.
During last 24 hours the geomagnetic conditions were at quiet to unsettled levels (NOAA KP 1-3, K Bel 1-3). Geomagnetic conditions are expected to be at unsettled levels, with isolated active periods possible on August 20 due to the ongoing high speed stream influence.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next days.
The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain below this threshold on August 20 and is likely to increase on August 21 and 22. The 24 hour electron fluence was at nominal levels. The electron fluence is expected to be at nominal levels for the next days.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 107, gebaseerd op 25 stations.
| Wolfgetal Catania | /// |
| 10cm zonneflux | 151 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 012 |
| Geschatte Ap | 010 |
| Geschat internationaal zonnevlekkengetal | 134 - Gebaseerd op 23 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
<< 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 | 08/12/2025 | X1.1 |
| Laatste M-klasse uitbarsting | 12/12/2025 | M1.1 |
| Laatste geomagnetische storm | 12/12/2025 | Kp5 (G1) |
| Zonnevlekkenloze dagen | |
|---|---|
| Laatste zonnevlekkenloze dag | 08/06/2022 |
| Maandelijks gemiddeld zonnevlekkengetal | |
|---|---|
| november 2025 | 91.8 -22.8 |
| december 2025 | 144.3 +52.5 |
| Afgelopen 30 dagen | 107.5 +8.8 |