Datum verslag: 2020 Apr 29 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
29 Apr 2020 | 069 | 006 |
30 Apr 2020 | 069 | 007 |
01 May 2020 | 069 | 009 |
Solar X-ray flux remained below B level. Active Regions (ARs) 2760 and 2761 decayed and not shown any significant flaring activity. Another small bipolar region with an associated sunspot, located around N22W38 has also emerged on Apr 29. Solar flaring activity is expected to remain at very low levels.
No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery in the last 24 hours.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to stay at nominal levels for the next 24 hours. The greater than 2 MeV electron flux was between nominal and moderate levels over the past 24 hours and is expected to be at nominal to moderate levels over the next 24 hours.
The solar wind speed near Earth decreased from around 430 km/s to 350 km/s and the total magnetic field varied between 1 and 6 nT (DSCOVR) over the past 24 hours. The Interplanetary Magnetic Field (IMF) was predominantly oriented towards the Sun (phi angle in the negative sector), with an extended deviation into the positive sector between 12 and 18 UT on Apr 28. Bz was mostly negative, with a minimum value of around -3 nT. Nominal solar wind conditions are expected for Apr 29 - May 01. The filament eruption observed on April 27 that possibly had an Earth directed component may be seen at Earth on May 02.
Geomagnetic conditions were quiet (local K Dourbes and NOAA Kp recorded values between 0-2). Quiet geomagnetic conditions are expected for Apr 29 - May 01 with isolated unsettled episodes possible due the patchy positive coronal hole that began to traverse the central meridian on Apr 26.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 024, gebaseerd op 15 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 069 |
AK Chambon La Forêt | 008 |
AK Wingst | 007 |
Geschatte Ap | 006 |
Geschat internationaal zonnevlekkengetal | 011 - Gebaseerd op 20 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 | 19/06/2025 | X1.9 |
Laatste M-klasse uitbarsting | 06/09/2025 | M1.2 |
Laatste geomagnetische storm | 16/09/2025 | Kp5 (G1) |
Zonnevlekkenloze dagen | |
---|---|
Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
---|---|
augustus 2025 | 133.5 +7.9 |
september 2025 | 109.4 -24.1 |
Afgelopen 30 dagen | 119.8 -10.9 |