Datum verslag: 2024 Oct 18 1231 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
18 Oct 2024 | 172 | 012 |
19 Oct 2024 | 175 | 017 |
20 Oct 2024 | 175 | 007 |
Solar flaring activity was low over the past 24 hours. The largest flare was a C6.6-flare, with peak time 14:27 UTC on October 17 2024, from SIDC Sunspot Group 290 NOAA AR 3860 (beta). There are currently 8 numbered active regions on the visible disk. SIDC Sunspot group 285 (NOAA AR 3856) is the most complex AR (beta-gamma-delta).The solar flaring activity is expected to be at moderate levels over the coming day with C-class flares expected and M-class flares probable and a chance of X-class flares.
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.
The small equatorial positive polarity mid-latitude coronal hole crossed the central meridian. A high-speed stream from this coronal hole may enhance the solar wind environment near Earth on October 21.
The solar wind at the Earth is slow. The solar wind speed decreased from around 400 km/s to 370 km/s and interplanetary magnetic field around 8 nT with the Bz reaching a minimum value of -7 nT. No enhancement of the solar wind speed and magnetic field is expected in the next 24h.
Geomagnetic conditions were quiet to unsettled (both NOAA Kp and local K Belgium 3) over the past 24 hours. Quiet conditions are expected in the next 24 hours.
The greater than 10 MeV proton flux remained below the 10 pfu threshold and is expected to remain so over the next days.
The greater than 2 MeV electron flux as measured by GOES 18 was shortly above the 1000 pfu alert threshold on OCT17 21:30 UTC, and has a small chance to exceed this level again shortly during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 126, gebaseerd op 08 stations.
Wolfgetal Catania | 179 |
10cm zonneflux | 174 |
AK Chambon La Forêt | 017 |
AK Wingst | 010 |
Geschatte Ap | 010 |
Geschat internationaal zonnevlekkengetal | 143 - Gebaseerd op 20 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
17 | 0212 | 0222 | 0238 | ---- | M1.0 | 54/3856 | II/1 | ||
17 | 0453 | 0505 | 0513 | S10W53 | M2.4 | SF | 42/3852 |
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 | 06/04/2025 | Kp5 (G1) |
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 |