Datum verslag: 2022 Oct 21 1248 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
21 Oct 2022 | 116 | 010 |
22 Oct 2022 | 135 | 005 |
23 Oct 2022 | 150 | 018 |
Solar flaring activity was at low levels, with flare of largest X-ray output being the C5.9-class flare, possibly from the rotated NOAA Active Region (AR) 3122, peak time 20 October 16:53 UTC. The two active regions present on the visible solar disk have remained mainly stable. For the next 24 hours, C-class flares are expected while M-class flares are possible.
A possibly Earth-directed Coronal Mass Ejection was observed in Lasco/C2 data on 21 October 04:49 UTC. This is believed to be associated with a radio pulse on 21 October 04:08 UTC and a C1.6-class flare, peak time 21 October 04:32 UTC from NOAA active region 3126 as well as an EUV wave. A possible impact on Earth may be expected 27 October 04:59 UTC, with the caveat that the CME speed is rather low and said impact may not be too profound.
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 reached the 1000 pfu alert threshold at 20 October 13:50 UTC. It can be expected be about threshold during the next 24 hours. The 24h electron fluence was at nominal levels over the past 24 hours and is expected to remain at this level in the next 24 hours.
Over the past 24 hours, the SW speed gradually ranged from 350 to 490 km/s. The total magnetic field (Bt) had values from 3 to 6 nT, while its Bz component fluctuated between -6 to 5 nT. The interplanetary magnetic field phi angle was predominately on the negative sector (directed towards the Sun). Over the next 24 hours, the solar wind parameters are not expected to become greatly enhanced from current levels.
Geomagnetic conditions were active locally on 20 October 16:00 UTC (K Dourbes 4). In the next 24 hours the conditions are expected to be quiet to unsettled, with a slight chance of active conditions.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 051, gebaseerd op 13 stations.
Wolfgetal Catania | 047 |
10cm zonneflux | 116 |
AK Chambon La Forêt | 013 |
AK Wingst | 008 |
Geschatte Ap | 007 |
Geschat internationaal zonnevlekkengetal | 032 - Gebaseerd op 26 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!
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 02:59 UTC
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 20:47 UTC
Het OVATION-model voorspelt dat het hemisferisch vermogen 101GW zal bereiken om 17:58 UTC
Het OVATION-model voorspelt dat het hemisferisch vermogen 75GW zal bereiken om 16:59 UTC
Het OVATION-model voorspelt dat het hemisferisch vermogen 51GW zal bereiken om 16:09 UTC
Laatste X-klasse uitbarsting | 19/06/2025 | X1.9 |
Laatste M-klasse uitbarsting | 30/08/2025 | M2.7 |
Laatste geomagnetische storm | 02/09/2025 | Kp5+ (G1) |
Zonnevlekkenloze dagen | |
---|---|
Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
---|---|
juli 2025 | 125.6 +9.3 |
september 2025 | 170 +44.4 |
Afgelopen 30 dagen | 138.6 +18.4 |