Datum verslag: 2021 Apr 03 1312 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
03 Apr 2021 | 074 | 005 |
04 Apr 2021 | 074 | 007 |
05 Apr 2021 | 074 | 014 |
The solar activity has been quiet over the past 24 hours. The visible solar disc is spotless and the X-ray flux is below B-level. The solar activity is expected to remain at low levels over the next 24 hours.
No Earth-directed coronal mass ejections (CMEs) was observed in the available coronagraph imagery.
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 exceeded 1000 pfu threshold on April 02, between 17:15 UTC and 17:40 UTC. It is expected to remain mainly below the 000 pfu threshold during the next 24 hours. The 24h electron fluence was at nominal levels in the last 24 hours and is expected to stay at normal levels for the next 24 hours.
The solar wind parameters (ACE and DSCOVR) were slightly enhanced due to the influence of the speed streams associated with small patchy equatorial coronal holes (in the south hemisphere, with negative polarity): The solar wind speed ranged between 349 km/s and 409 km/s . The interplanetary magnetic field magnitude peaked at 9.0 nT, and Bz components varied between -7.5 nT and 6.6 nT. The high-speed streams associated with the equatorial coronal hole (positive magnetic polarity and facing Earth on March 31) is expected to slightly enhanced the solar wind conditions near Earth later today and tomorrow on April 3 and 4. A large equatorial coronal hole (with a positive magnetic polarity) is currently facing Earth. The high-speed stream associated with this coronal hole is expected to reach Earth in about 3 days.
Geomagnetic conditions were quiet to unsettle (Kp and K-Dourbes: 1-3) due to the slight enhancement of the solar wind conditions. Quiet to unsettled conditions is expected to persist followed by possible periods of active conditions on April 2, due to the expected influence of the high-speed streams associated with the equatorial coronal hole (facing Earth on March 31).
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 000, gebaseerd op 18 stations.
Wolfgetal Catania | 000 |
10cm zonneflux | 072 |
AK Chambon La Forêt | 011 |
AK Wingst | 007 |
Geschatte Ap | 006 |
Geschat internationaal zonnevlekkengetal | 000 - Gebaseerd op 32 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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Zonnevlekkenloze dagen | |
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Laatste zonnevlekkenloze dag | 08/06/2022 |
Maandelijks gemiddeld zonnevlekkengetal | |
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