Datum verslag: 2023 Aug 18 1241 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 18 Aug 2023 | 153 | 013 |
| 19 Aug 2023 | 151 | 014 |
| 20 Aug 2023 | 148 | 008 |
The solar flaring activity was at low levels. The largest flare was a C5.1 flare peaking at 12:40 UTC on August 17, this originated near the west limb associated with NOAA AR3397, which has now rotated over the limb. NOAA AR 3403 decayed over the period and was quiet. NOAA AR3405 also produced C-class flares and has been split into two regions including the small new region NOAA AR3411. NOAA AR3407 and AR3410 were stable and quiet. NOAA ARs 3406, 3408 both decayed into plage region. NOAA AR3409, which began to emerge yesterday has continued to grow and produced low level C-class flares. The solar flaring activity is expected to be at low levels over the next 24 hours with C-class flares likely and a low chance for isolated M-class flares.
There were no Earth-directed Coronal Mass Ejections (CMEs) detected in the available coronagraph observations.
The solar wind parameters reflected a weak negative polarity high speed stream arrival. The interplanetary magnetic field was slightly enhanced, with a significant increase around 02:00 UTC on August 18, when it jumped from 9 and 14 nT. Bz had a minimum value of -11nT. The solar wind speed increased gradually from 02:00 UTC, from 300km/s to values near 500 km/s. The interplanetary magnetic field orientation switched to the negative sector (field directed towards the Sun) from 19:00 UTC on August 17. The solar wind parameters are expected to remain enhanced on August 18 and 19, while the Earth remains under the influence for the high-speed stream.
During last 24 hours the geomagnetic conditions were at quiet to unsettled levels (NOAA KP 1-3 and K-Bel 1-3). Geomagnetic conditions are expected to be at unsettled levels, with active periods possible on August 18 and 19, due to the ongoing high speed stream influence.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next days.
The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain below this threshold over the next days. The 24 hour electron fluence was at nominal levels. The electron fluence is expected to be at nominal levels for the next days.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 125, gebaseerd op 14 stations.
| Wolfgetal Catania | /// |
| 10cm zonneflux | 152 |
| AK Chambon La Forêt | 011 |
| AK Wingst | 010 |
| Geschatte Ap | 009 |
| Geschat internationaal zonnevlekkengetal | 149 - Gebaseerd op 24 stations |
| Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Geen | ||||||||||
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!
| Laatste X-klasse uitbarsting | 01/12/2025 | X1.9 |
| Laatste M-klasse uitbarsting | 08/12/2025 | M2.0 |
| Laatste geomagnetische storm | 04/12/2025 | Kp5 (G1) |
| Zonnevlekkenloze dagen | |
|---|---|
| Laatste zonnevlekkenloze dag | 08/06/2022 |
| Maandelijks gemiddeld zonnevlekkengetal | |
|---|---|
| november 2025 | 91.8 -22.8 |
| december 2025 | 167.7 +75.9 |
| Afgelopen 30 dagen | 107.1 +12.4 |