Datum verslag: 2021 May 23 1231 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
23 May 2021 | 076 | 007 |
24 May 2021 | 076 | 007 |
25 May 2021 | 076 | 012 |
NOAA AR 2824 (Catania 96) has grown significantly in complexity over the last 24 hours, it has now a beta-gamma magnetic field configuration and it has produced three M-class flares and numerous C-class flares. The strongest one was an M1.4 flare, peaking at 21:36 UT on 22 May. More M-class flares can be expected.
Three (partially) Earth directed CMEs erupted on 22 May. Two of them are associated with M-class flares. The first one starting at 09:12 UT (LASCO C2) with 300 km/s and about 90 degrees angular width, expected arrival at 23 UT on 26 May. The second one at 16:23 UT (COR2A), with a speed of 460 km/s and an expected arrival time at 02 UT on 26 May. The last one started at 22:00 UT (COR2A), with a speed of 629 km/s, and expected to arrive at 13 UT on 25 May. The last two were faint in LASCO and better visible in COR2. The speed of the CMEs increased from the first to the third, so they will encounter and interact on their way to the Earth, making accurate arrival time predictions difficult.
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 remained barely below the 1000 pfu in the past 24 hours, it is expected to decrease in the coming 24 hours. The 24-hour electron fluence was at normal levels in the past 24 hours, but close to the moderate limit, it may reach this level before decreasing in the coming 24 hours.
The solar wind speed at the Earth has been around 420 km/s over the past 24 hours, with interplanetary magnetic field magnitude around 3 nT. The polarity of the magnetic field was mostly negative (towards the Sun). Similar conditions are expected for the next 24 hours.
Geomagnetic conditions have been quiet (KDourbes 1-2, Kp 1-2), similar conditions can be expected for the next 24 hours.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 026, gebaseerd op 15 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 076 |
AK Chambon La Forêt | 010 |
AK Wingst | 006 |
Geschatte Ap | 005 |
Geschat internationaal zonnevlekkengetal | 017 - Gebaseerd op 26 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
22 | 1703 | 1711 | 1716 | N17E20 | M1.1 | 1N | 17 | 96/2824 | III/2 |
22 | 2130 | 2136 | 2143 | N19E15 | M1.4 | 1N | 40 | 96/2824 | |
23 | 1100 | 1108 | 1114 | N18E10 | M1.1 | SF | 85 | 96/2824 | 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
Op basis van de huidige parameters is er in de nabije toekomst een beperkte kans op poollicht op de volgende locaties van de gemiddelde breedtegraad
Surgut, YakutskOm 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: 13:07 UTC
Het OVATION-model voorspelt dat het hemisferisch vermogen 75GW zal bereiken om 13:21 UTC
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 23:59 UTC
G1 - Kleine geomagnetische storm (Kp5) Drempel bereikt: 20:02 UTC
Het OVATION-model voorspelt dat het hemisferisch vermogen 50GW zal bereiken om 13:56 UTC
Laatste X-klasse uitbarsting | 28/03/2025 | X1.1 |
Laatste M-klasse uitbarsting | 01/04/2025 | M2.5 |
Laatste geomagnetische storm | 27/03/2025 | Kp5 (G1) |
Zonnevlekkenloze dagen | |
---|---|
Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
---|---|
maart 2025 | 134.2 -20.4 |
april 2025 | 143 +8.8 |
Afgelopen 30 dagen | 130.4 -16.1 |