Datum verslag: 2021 Apr 29 1234 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
29 Apr 2021 | 078 | 006 |
30 Apr 2021 | 077 | 014 |
01 May 2021 | 076 | 031 |
X-ray flux has remained below C level throughout the period. All three regions on disc remained stable or in decay. Both Catania groups 91 and 92 (NOAA regions 2821 and 2820) decreased in size. X-ray flux is likely to remain below C level though an isolated C-flare is still possible.
No new Earth directed CMEs have been detected in coronagraph data.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux just touched the 1000 pfu event threshold. The 24h electron fluence was at normal levels but rising. As Solar wind enhancements have dyed out, the electron fluence is expected to remain at normal levels during next days.
Earth is within a slow Solar wind regime. Solar wind speed is stable at around 320km/s since midnight while total magnetic field was under 5nT with an unremarkable Bz component and a phi angle indicating magnetic field orientation towards the Sun. By end of tomorrow April 30, start of May 1 we may see Solar wind perturbations due to a combination of enhanced speed associated to the positive polarity coronal hole that transited the central meridian in the past days, and magnetic field perturbations due to passing magnetic clouds from first the April 25 CME and later the April 26 CME. Though likelihood and confidence for the CME arrivals is low.
Geomagnetic conditions were quiet (local K Dourbes and NOAA Kp 0-2). Geomagnetic conditions are expected to be quiet to unsettled and then possibly increasing late tomorrow to active conditions with also minor storm levels possible if any of the CME arrivals show up.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 037, gebaseerd op 09 stations.
Wolfgetal Catania | 050 |
10cm zonneflux | 078 |
AK Chambon La Forêt | 006 |
AK Wingst | 002 |
Geschatte Ap | 002 |
Geschat internationaal zonnevlekkengetal | 043 - Gebaseerd op 25 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
Op basis van de huidige parameters is er in de nabije toekomst een beperkte kans op poollicht op de volgende locaties van de hoge breedtegraad
Iqaluit, NUOm ook bereikbaar te blijven bij grote poollichtkansen hebben we een zware server nodig die alle bezoekers aankan. Doneer en steun dit project zodat we online blijven en je geen enkele poollichtkans mist!
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 01:50 UTC
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 20:20 UTC
Matige M1.05 zonnevlam
Kleine R1 radio blackout gedetecteerd (≥M1 - momenteel: M1.05)
Het OVATION-model voorspelt dat het hemisferisch vermogen 78GW zal bereiken om 10:32 UTC
Laatste X-klasse uitbarsting | 28/03/2025 | X1.1 |
Laatste M-klasse uitbarsting | 05/04/2025 | M1.0 |
Laatste geomagnetische storm | 05/04/2025 | Kp6- (G2) |
Zonnevlekkenloze dagen | |
---|---|
Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
---|---|
maart 2025 | 134.2 -20.4 |
april 2025 | 150.4 +16.2 |
Afgelopen 30 dagen | 132.4 -10.1 |