Datum verslag: 2020 May 03 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
03 May 2020 | 069 | 003 |
04 May 2020 | 068 | 008 |
05 May 2020 | 068 | 010 |
Solar flaring activity was at very low levels. No significant flares have been recorded. Solar 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 oscillated around 320 km/s (DSCOVR). The total magnetic field was unremarkable, varying between 0 and 7 nT. Bz reached a minimum of -4 nT. The Interplanetary Magnetic Field (IMF) phi angle was predominantly in the negative sector (directed towards the Sun). Predominantly background solar wind conditions are expected for May 03 - 05. The solar wind associated with the negative polarity coronal hole, that transited the central meridian on May 01, is predicted to influence Earth from late on May 04.
Geomagnetic conditions were quiet (local K Dourbes and NOAA Kp recorded values between 0-2) over the last 24 hours. Quiet geomagnetic conditions are expected for May 03 with unsettled conditions possible from late on May 04, due to the arrival of the high speed stream associated with the small equatorial coronal hole mentioned above.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 000, gebaseerd op 16 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 069 |
AK Chambon La Forêt | 008 |
AK Wingst | 006 |
Geschatte Ap | 005 |
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
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
Gillam, MB, 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 |