Datum verslag: 2021 Nov 14 1232 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
14 Nov 2021 | 079 | 004 |
15 Nov 2021 | 077 | 004 |
16 Nov 2021 | 078 | 005 |
The solar activity was at very low levels over the past 24 hours with low B-class flaring. Active region NOAA 2895 has now rotated behind the west limb. NOAA 2894 has undergone a decay, losing its trailing spot, and is now classified as magnetic-type beta. It has been inactive and so was NOAA 2893 (alpha). The solar activity is expected to be at very low to low levels with a slight chance for C-class flaring from NOAA 2894 over the next 24 hours.
No Earth-directed coronal mass ejections (CMEs) were observed in the available coronagraph imagery.
Over the past 24 hours the greater than 10 MeV proton flux was at background levels and is expected to remain so in the next 24 hours. The greater than 2MeV electron has shortly crossed the 1000 pfu threshold and might briefly cross the 1000 pfu threshold again in the next 24 hours. The 24h electron fluence was at the border of nominal to moderate levels and is expected to remain so in the next 24 hours.
Over the past 24 hours the solar wind parameters (ACE and DSCOVR) remained at background slow solar wind conditions. The solar wind speed varied between 299 km/s and 360 km/s. The interplanetary magnetic field was weak with a maximum of 5.5 nT. The north-south Bz component varied between -4.5 nT and 3.6 nT. The interplanetary magnetic remained predominantly in the negative sector. The solar wind parameters are expected to remain at background solar wind conditions over the next 24 hours.
The geomagnetic conditions over the past 24 hours were quiet and are expected to remain mostly quiet until Nov 17th. Then unsettled to active conditions with possible minor storm intervals are expected due to a foreseen high speed stream arrival from a large negative-polarity mid- latitude coronal hole, which crossed the central meridian last night.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 021, gebaseerd op 08 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 081 |
AK Chambon La Forêt | 005 |
AK Wingst | 002 |
Geschatte Ap | 002 |
Geschat internationaal zonnevlekkengetal | 025 - Gebaseerd op 16 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
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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 | |
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Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
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maart 2025 | 134.2 -20.4 |
april 2025 | 148.7 +14.5 |
Afgelopen 30 dagen | 132.7 -9.9 |