Datum verslag: 2020 Jan 10 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Proton event expected (10 pfu at >10 MeV)
| 10cm flux | Ap | |
|---|---|---|
| 10 Jan 2020 | 074 | 008 |
| 11 Jan 2020 | 074 | 007 |
| 12 Jan 2020 | 074 | 007 |
The solar activity has been at low levels over the past 24 hours. Two small bipolar sunspots are currently visible on the disc: Catania sunspots group 26 (NOAA AR-2756) in the North-West quadrant of the Sun, and Catania sunspot group 27, whish is the region close to the equator that turned over the East limb on Jan 07 and produced a narrow coronal mass ejection. No significant flaring activity has been observed in these regions and the X-ray flux remained below C-level. The solar activity is expected to remain at low levels with a small chances of C-class flare and possibly slow coronal mass ejections for the next 24 hours.
No earth-directed coronal mass ejection was identified in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values.
The solar wind environment near Earth was under the influence of the coronal hole high-speed streams. The solar wind speed increased from 400 km/s to about 590 km/s, the total magnetic field fluctuated between 2 nT and 7.6 nT, and the southern component of the magnetic filed was between -6 nT and 5.3 nT (as recorded by the ACE spacecraft). Currently the solar wind speed is decreasing and ranges around 500 km/s. We expect the solar wind parameters to return slowly towards an ambient background and slow solar wind speed regime in the next two days. An extension to the North Polar coronal hole (positive polarity), and a positive polarity equatorial coronal hole reached the central meridian today. The high-speed stream coming from those two coronal holes is expected to enhance the solar wind environment near Earth in more than 2-3 days from now.
Quiet to unsettled geomagnetic conditions were observed in response to the solar wind enhancement. Quiet to unsettle conditions is expected for the next 24 hours.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 000, gebaseerd op 16 stations.
| Wolfgetal Catania | 016 |
| 10cm zonneflux | 074 |
| AK Chambon La Forêt | 016 |
| AK Wingst | 012 |
| Geschatte Ap | 012 |
| Geschat internationaal zonnevlekkengetal | 015 - Gebaseerd op 18 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 | 150 +58.2 |
| Afgelopen 30 dagen | 108.8 +10.3 |