Datum verslag: 2023 May 03 1253 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
03 May 2023 | 157 | 002 |
04 May 2023 | 157 | 001 |
05 May 2023 | 157 | 001 |
Solar flaring activity was at moderate levels over the past 24 hours with several M-class flare. While NOAA Active Region 3288 located close to the west limb decayed and produced only few C-class flare, the NOAA Active Region 3293 has been growing and has produced all the recent M-class flares. The larger flare was an M7.1 peaking today at 10:45 UTC. The flaring activity is expected to remain moderate with possible M-class flare and a small chance of X-class flare.
Few coronal mass ejections (CME) and flows were observed in the available SOHO/LASCO coronagraph imagery and automatically detected by the Cactus tool over the past 24 hours. However, no clear Earth-directed coronal mass ejections were identified.
The greater than 10 MeV proton flux was at the background levels over the past 24 hours. The proton flux is expected to remain at the background levels over the next day, with a very small chance that a particle event occurs in association with an X-class flare. The greater than 2 MeV electron flux was above the 1000 pfu threshold due to the enhanced solar wind conditions and is expected to remain at that level over the next day. The 24-hour electron fluence was at moderate levels and is expected to remind at moderate levels over the next 24 hours.
The influence of the solar wind streams associated to the negative polarity coronal hole has decreased to return to a slow solar wind regime. The solar wind speed decreased from 530 km/s to 440 km/s. The total interplanetary magnetic showed the values below 6.0 nT, and the southward interplanetary magnetic component, Bz, fluctuated between -3.1 nT and 4.7 nT. The solar wind conditions near Earth is expected to remain within the slow solar wind regime for the next 24 hours.
Geomagnetic conditions were mostly quiet with some very short periods of unsettle conditions observed by the local stations (NOAA-Kp: 0 to 2, and K-BEL: 0 to 3). For the next 24 hours,the geomagnetic conditions are expected to remain quiet with possible short periods of unsettle conditions.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 120, gebaseerd op 17 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 157 |
AK Chambon La Forêt | 009 |
AK Wingst | 009 |
Geschatte Ap | 010 |
Geschat internationaal zonnevlekkengetal | 119 - Gebaseerd op 27 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
03 | 0915 | 0927 | 0933 | N14E44 | M4.2 | 1B | --/3293 | ||
03 | 1003 | 1014 | 1019 | ---- | M3.1 | --/3293 |
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
TórshavnOm 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 |