Datum verslag: 2015 Jun 19 1230 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
19 Jun 2015 | 150 | 008 |
20 Jun 2015 | 150 | 007 |
21 Jun 2015 | 150 | 046 |
Solar flaring activity was moderate with a long duration M3.0 flare originating from Catania group 92 (NOAA 2371) peaking around 17:36UT. It was associated with a dimming and an EUV wave and a corresponding asymmetric halo in SoHO/LASCO coronagraph images. Several further C flares were recorded from Catania groups 92 (including a C8.1 flare peaking at 9:27UT) as well as 87 (NOAA 2371 and 2367 respectively). Catania group 92 has a complex beta-gamma-delta configuration while also Catania group 87 deserves continued attention. Flaring at M level is likely for the next days from those two sources. The 10 MeV proton flux remained above the event threshold for most of the afternoon of June 18. Since around midnight flux values are below the event threshold and further declining. The asymmetric full halo CME associated to the M3.0 flare is visible in SoHO/LASCO data, from 17:24 UT (June 18) onwards in the C2 field of view. The bulk of the mass is expelled in Eastern direction off the Sun-Earth line (with the source region located at longitude -45 degrees approximately at the time of the event) with a projected speed of around 1000km/s (Cactus software is underestimating the speed). Impact of this CME on Earth is currently expected before UT noon June 21. Another CME is visible in SoHO/LASCO C2 data from 8:25UT onwards (after a datagap). It is directed predominantly southward and associated with a filament eruption in the south-east quadrant. We await further data for assessment of possible Earth-directed CME component. Solar wind conditions are gradually further restoring to nominal. Solar wind speed decreased from around 420 km/s to around 370 km/s. total magnetic field was in the 4-5nT range with variable Bz. Geomagnetic conditions were quiet to unsettled (NOAA Kp 1-3, local K Dourbes 0-3). Quiet geomagnetic conditions are expected over the next 24-36 hours, with afterwards the likely impact of the June 18 17:24UT CME arriving around or before noon June 21 with possible associated geomagnetic storm conditions.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 053, gebaseerd op 06 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 151 |
AK Chambon La Forêt | 012 |
AK Wingst | 010 |
Geschatte Ap | 010 |
Geschat internationaal zonnevlekkengetal | 063 - Gebaseerd op 23 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
18 | 0033 | 0127 | 0155 | ---- | M1.2 | 85/2365 | CTM/1VI/1 | ||
18 | 1630 | 1736 | 1825 | N15E50 | M3.0 | 1N | 2200 | 92/2371 | III/1IV/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 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 | 13/04/2025 | M2.2 |
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 |