Datum verslag: 2022 Aug 28 1233 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Aug 2022 | 128 | 019 |
29 Aug 2022 | 122 | 029 |
30 Aug 2022 | 126 | 013 |
Solar flaring activity was at moderate levels over the past 24 hours, with flare of largest X-ray output being a M1.4-class flare from NOAA AR 3088. The vast majority of the flaring activity was originated from said region, which developed further and is about to rotate off disk. A new region emerged on the visible solar disk on the NE quadrant. For the next 24 hours, C-class flares are expected while M-class flares are possible.
A filament eruption can be seen NW of NOAA AR 3089 at 27 August 18:25 UTC. This event will be monitored. No new Earth-directed CMEs were recorded over the past 24 hours.
The greater than 10 MeV proton flux decreased below the 10 pfu mark at 27 August 21:45 UTC. The proton flux is expected to continue decreasing over the next 24 hours. The greater than 2MeV electron flux was below the 1000 pfu threshold over the past 24 hours. It is expected to remain below threshold over the next 24 hours. The 24h electron fluence was at nominal levels over the past 24 hours. It is expected to remain at nominal levels over the next 24 hours.
The solar wind parameters reflected waning ICME and High Speed Stream (HSS) influences over the past 24 hours. The solar wind magnetic field values decreased from 14 to 2 nT, while Bz had values between -10 and 12 nT. The solar wind speed reached 525 km/s. The interplanetary magnetic field phi angle was predominantly on the negative sector (towards the Sun). Over the next 24 hours, a glancing blow from the CME of 27 August 02:12 UTC can be expected, as well as the HSS from the negative polarity southern coronal hole.
Active conditions were recorded over the past 24 hours (NOAA Kp and K Dourbes 4). Over the next 24 hours, unsettled to active conditions can be expected, while a minor storm event is possible.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 090, gebaseerd op 19 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 128 |
AK Chambon La Forêt | 021 |
AK Wingst | 012 |
Geschatte Ap | 013 |
Geschat internationaal zonnevlekkengetal | 098 - Gebaseerd op 29 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
27 | 1513 | 1525 | 1530 | S28W71 | M1.1 | SF | 21/3088 | ||
27 | 1545 | 1558 | 1621 | ---- | M1.8 | 21/3088 | CTM/1 | ||
28 | 0047 | 0134 | 0138 | ---- | M1.4 | 21/3088 |
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
Norilsk, VorkutaVeel 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!
Laatste X-klasse uitbarsting | 19/06/2025 | X1.9 |
Laatste M-klasse uitbarsting | 06/09/2025 | M1.2 |
Laatste geomagnetische storm | 09/09/2025 | Kp6- (G2) |
Zonnevlekkenloze dagen | |
---|---|
Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
---|---|
augustus 2025 | 133.5 +7.9 |
september 2025 | 109.6 -23.9 |
Afgelopen 30 dagen | 119.2 -19.8 |