Datum verslag: 2019 Mar 16 1236 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 16 Mar 2019 | 070 | 015 |
| 17 Mar 2019 | 069 | 022 |
| 18 Mar 2019 | 069 | 008 |
X-ray flux remained below B level. With a spotless disk, again X-ray flux is expected to remain below C level.
No new Earth directed CME's have been detected in coronagraph data.
The Solar proton flux levels were at background values and are expected to remain so.
Solar wind conditions continued to reflect the influence of the coronal hole, with Solar wind speed increasing but not reaching above current values of around 430 km/s. Total magnetic field reached a peak of just over 8nT late yesterday before decreasing steadily to current values between 5-6nT. Bz was variable in general but recently negative with values down below -5nT. The magnetic field phi angle was stable in the negative sector. Solar wind conditions will remain slightly enhanced with wind speed likely to rise somewhat further under the influence of the equatorial coronal hole, though speeds should start to decrease over the next 24 hours. Further slow transient perturbations are also possible in the next 24 hours due to the March 12 CME. Late March 18, early March 19 we are expected to see the influence of the equatorial positive polarity coronal hole that passed central meridian March 14/15.
Geomagnetic conditions were quiet to unsettled (NOAA Kp 0-3 and local K Dourbes 1-3). Geomagnetic conditions are expected to be quiet to unsettled with a possibility for active periods under enhanced solar speed speed conditions, possibly combined with some CME transients. Afterwards, geomagnetic conditions are expected to become quiet until the high speed stream expected late March 18, early March 19.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 000, gebaseerd op 09 stations.
| Wolfgetal Catania | 000 |
| 10cm zonneflux | 070 |
| AK Chambon La Forêt | 010 |
| AK Wingst | 009 |
| Geschatte Ap | 008 |
| Geschat internationaal zonnevlekkengetal | 000 - Gebaseerd op 15 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 |