Datum verslag: 2022 Oct 30 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
30 Oct 2022 | 131 | 011 |
31 Oct 2022 | 129 | 009 |
01 Nov 2022 | 122 | 017 |
Solar flaring activity was at low levels and infrequent, with two C1 flares detected over the last 24 hours. NOAA Active Regions (AR) 3130 (Catania group 72, magnetic type Beta) and 3133 (Catania group 76, magnetic type Beta) produced the C-class activity. Both AR show signs of a small decay but NOAA AR 3130 still has a chance to produce C-class activity. NOAA AR 3135 (magnetic type Beta) produced a B9 flare in the last 24 hours and remains magnetically complex, so C-flare activity from this location is still possible.
No Earth-directed Coronal Mass Ejections were observed 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 remain so for the next 24 hours. The greater than 2 MeV electron flux increased significantly during the last 24 hours, however, it remained below the 1000 pfu alert threshold and is expected to stay so during the next 24 hours. The 24h electron fluence also increased following the increase of the greater than 2 MeV electron flux, nevertheless, it remained at nominal levels and is expected to continue so for the next 24 hours.
The Solar Wind (SW) conditions are still affected by the arrival of a High Speed Stream (HSS), on 28 Oct. The SW speed varied between 510 to 610 km/h during the last 24 hours. The total magnetic field (Bt) was at low levels, between 2 and 7 nT, while its north-south component (Bz) fluctuated between -5 and 5 nT over the last 24 hours. The interplanetary magnetic field (phi) angle was predominantly positive (directed away from the Sun) during the last 24 hours. The SW conditions are expected to remain under the influence of the HSS for the next 24 hours, but with a gradual decrease in SW speed.
Geomagnetic conditions reached globally and locally active levels (NOAA Kp and K Belgium 2-4) over the last 24 hours. Quite conditions are expected for the next 24 hours both globally and locally (NOAA Kp and K Belgium up to 3), unless the HSS expected for the second half of 31 Oct arrives early.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 083, gebaseerd op 13 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 134 |
AK Chambon La Forêt | 035 |
AK Wingst | 026 |
Geschatte Ap | 030 |
Geschat internationaal zonnevlekkengetal | 081 - Gebaseerd op 16 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, Yellowknife, NTOm 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!
Matige M2.31 zonnevlam
Kleine R1 radio blackout gedetecteerd (≥M1 - momenteel: M1.89)
Matige M1.12 zonnevlam
Matige M1.13 zonnevlam
Kleine R1 radio blackout gedetecteerd (≥M1 - momenteel: M1.13)
Laatste X-klasse uitbarsting | 28/03/2025 | X1.1 |
Laatste M-klasse uitbarsting | 12/04/2025 | M1.3 |
Laatste geomagnetische storm | 06/04/2025 | Kp5 (G1) |
Zonnevlekkenloze dagen | |
---|---|
Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
---|---|
maart 2025 | 134.2 -20.4 |
april 2025 | 136.4 +2.2 |
Afgelopen 30 dagen | 134.7 -7.2 |