Datum verslag: 2023 Jan 06 1237 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
06 Jan 2023 | 159 | 005 |
07 Jan 2023 | 162 | 005 |
08 Jan 2023 | 164 | 003 |
Solar flaring activity reached high levels. NOAA Active Region (AR) 3182 produced an X1.2 flare, peaking at 00:57 UTC January 06. Further C-class flares were produced by NOAA ARs 3176, 3180, 3181 and a new active region NOAA 3183. NOAA AR 3183 emerged rapidly on January 05 in the southern hemisphere near the central meridian. NOAA AR 3181 showed further emergence and trailer sunspot development. NOAA AR 3137 showed signs of decay, while NOAA AR 3136 has rotated off the solar disk. Solar flaring activity is expected to be moderate over the next 24 hours with a high probability of C-class flares, M flares likely and a chance for further X-class flares.
No Earth directed CMEs have been observed in the coronagraph data.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux was below the 1000 pfu threshold. It is expected remain below the 1000 pfu threshold over the next 24 hours. The electron fluence was at normal levels and is expected to be at normal levels over the next days.
The magnitude of the interplanetary magnetic field gradually decreased from 17nT to a minimum of 6 nT at 00 UTC. The values then increased again slightly and were around 10nT for the second half of the period. The orientation of the magnetic field was predominantly in the negative sector (field directed towards from the Sun). The Bz was negative for a sustained period between 12 and 22 UTC January 05, before becoming mostly positive (Bz had a minimum of -10nT). The solar wind speed values gradually increased from 18 UTC on January 5, with maximum value of 550 km/s. The magnetic field magnitude is expected to continue to slowly. January 07-08 we expected a gradual return to slow solar wind regime.
Geomagnetic conditions were quiet to unsettled (NOAA Kp and local K-Dourbes reached 3). Unsettled conditions are expected with possible isolated active conditions still be possible on January 06 and 07.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 132, gebaseerd op 10 stations.
Wolfgetal Catania | 120 |
10cm zonneflux | 154 |
AK Chambon La Forêt | 015 |
AK Wingst | 011 |
Geschatte Ap | 009 |
Geschat internationaal zonnevlekkengetal | 110 - Gebaseerd op 18 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
06 | 0043 | 0057 | 0107 | S18E68 | X1.2 | 2B | 420 | 38/3182 | III/2 |
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!
Het OVATION-model voorspelt dat het hemisferisch vermogen 50GW zal bereiken om 02:13 UTC
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 19:16 UTC
Actieve geomagnetische condities (Kp4) Drempel bereikt: 14:16 UTC
Matige M1.13 zonnevlam
Kleine R1 radio blackout gedetecteerd (≥M1 - momenteel: M1.03)
Laatste X-klasse uitbarsting | 19/06/2025 | X1.9 |
Laatste M-klasse uitbarsting | 19/08/2025 | M1.1 |
Laatste geomagnetische storm | 09/08/2025 | Kp6 (G2) |
Zonnevlekkenloze dagen | |
---|---|
Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
---|---|
juli 2025 | 125.6 +9.3 |
augustus 2025 | 128.8 +3.2 |
Afgelopen 30 dagen | 127 +11.7 |