Datum verslag: 2020 Mar 08 1233 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 08 Mar 2020 | 070 | 006 |
| 09 Mar 2020 | 070 | 008 |
| 10 Mar 2020 | 070 | 011 |
The solar activity was at low levels over the past 24 hours with the X-ray flux below B-level. A newly emerged sunspot is visible on the solar disc in the South-East quadrant. This sunspot is not numbered by NOAA and Catatonia yet. The solar activity is expected to remain at low levels for the next 24 hours with a small chance of C-class flare from the newly emerge sunspots.
No earth-directed coronal mass ejections (CMEs) have been identified in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values.
The high-speed streams from the south polar coronal hole continued to slightly influence the solar wind environment near Earth. The solar wind parameters show mostly slow solar wind speed regime with minor enhancement: the solar wind speed ranged between 330 km/s and 400 km/s with a peak of about 414 km/s around 04:00 UTC (on March 08), the total interplanetary magnetic field ranged between 2.3 nT and 7.1 nT, and the southward component fluctuated between -3.9 nT and 6.9 nT. The solar wind environment is expected to remain mostly in the slow wind speed regime with some minor enhancements due to the influence of the south polar coronal hole high- speed streams. The southern polar coronal hole shows an extension reaching 30 degree latitude south, which is currently facing Earth. The high-speed streams coming from that extension will influence the solar wind condition near Earth by further enhancing the solar wind parameters in about 3 days from now.
The geomagnetic conditions were quiet with few periods of unsettled condition observed by Dourbes station (K-Dourbes = 3). We expect the geomagnetic conditions to remain mostly quiet with possible periods of unsettled condition.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 014, gebaseerd op 17 stations.
| Wolfgetal Catania | /// |
| 10cm zonneflux | 070 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 004 |
| Geschatte Ap | 004 |
| Geschat internationaal zonnevlekkengetal | 000 - Gebaseerd op 28 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 | 10/12/2025 | M4.4 |
| Laatste geomagnetische storm | 10/12/2025 | Kp6+ (G2) |
| Zonnevlekkenloze dagen | |
|---|---|
| Laatste zonnevlekkenloze dag | 08/06/2022 |
| Maandelijks gemiddeld zonnevlekkengetal | |
|---|---|
| november 2025 | 91.8 -22.8 |
| december 2025 | 155.3 +63.5 |
| Afgelopen 30 dagen | 109 +10.8 |