Datum verslag: 2026 Aug 07 1234 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 07 Aug 2026 | 096 | 011 |
| 08 Aug 2026 | 095 | 025 |
| 09 Aug 2026 | 100 | 008 |
Solar flaring activity was low over the past 24 hours. The largest flare was a C1.0 flare (SIDC Flare 8337) peaking on August 06 at 19:29 UTC. There are currently 4 numbered regions on the disk. All the regions are simple and either stable or in decay. Solar flaring activity is expected to be low over the next 24 hours.
No new Earth directed Coronal Mass Ejections (CMEs) were detected in the available coronagraph imagery.
Over the past 24 hours, the solar wind parameters reflected a slow solar wind regime. The magnetic field strength ranged between 1 and 6 nT. The solar wind speed decreased from 310 km/s to around 360 km/s. The solar wind conditions are expected to continue to reflect slow solar wind conditions on August 07, with possible weak enhancements due to any glancing blow from the CMEs from August 03. Further enhancements are possible on August 08 due to a glancing blow CME arrival from August 04 and CIR influence.
Geomagnetic conditions were at quiet levels (NOAA KP and K Bel 1 to 2). Quiet conditions are expected on August 07 with possible active intervals in response to any glancing blow from the CMEs from August 03. Active to minor storm conditions are possible on August 08 due to CME arrival from August 04 and CIR.
The greater than 10 MeV proton flux was below the 10 pfu threshold over the past 24 hours. It is expected to remain below this threshold level over the next 24 hours.
The greater than 2 MeV electron flux, as measured by GOES-18 and GOES-19, was below the 1000 pfu threshold. The greater than 2 MeV electron flux is expected to be below this threshold over the next 24 hours. The electron fluence was at normal levels and is expected to be at normal levels for the next 24 hours.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 055, gebaseerd op 16 stations.
| Wolfgetal Catania | 083 |
| 10cm zonneflux | 101 |
| AK Chambon La Forêt | 003 |
| AK Wingst | 002 |
| Geschatte Ap | 002 |
| Geschat internationaal zonnevlekkengetal | 057 - Gebaseerd op 32 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 | 04/07/2026 | X1.3 |
| Laatste M-klasse uitbarsting | 05/09/2026 | M1.0 |
| Laatste geomagnetische storm | 08/09/2026 | Kp5 (G1) |
| Zonnevlekkenloze dagen | |
|---|---|
| Afgelopen 365 dagen | 4 dagen |
| 2026 | 4 dagen (2%) |
| Laatste zonnevlekkenloze dag | 18/09/2026 |
| Maandelijks gemiddeld zonnevlekkengetal | |
|---|---|
| augustus 2026 | 76 -2.1 |
| september 2026 | 64 -12 |
| Afgelopen 30 dagen | 70.2 -18 |