Datum verslag: 2023 Apr 05 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
05 Apr 2023 | 135 | 011 |
06 Apr 2023 | 133 | 008 |
07 Apr 2023 | 130 | 005 |
Despite the presence of the complex NOAA AR 3270 on the visible side of the solar disc (classified yesterday as the beta-gamma-delta region), the solar flaring activity was during last 24 hours very low with only few B-class and low C-class flares reported. The NOAA AR 3270 shows decrease in complexity and it has now beta-gamma configuration of the photospheric magnetic field. We expect a low level of flaring activity to persist in the coming hours with C-class flares, while isolated M-class flares are possible but not very probable.
During last 24 hours there were no potentially Earth-directed CMEs detected in the coronagraph observations.
The greater than 10 MeV proton flux remained at the background levels, and the greater than 2 MeV electron flux was fluctuating around the 1000 pfu threshold, we expect both of these parameters will stay on the similar level in the coming hours. The 24h electron fluence is still at moderate to normal level, and we expect it to decrease to the normal level until tomorrow.
Earth is still withing the rather fast solar wind. During last 48 hours the solar wind velocity was fluctuating between about 530 and 490 km/s, with the present value around 480 km/s. The interplanetary magnetic field magnitude is around 5 nT.
During last 24 hours the geomagnetic conditions were quiet to unsettled (NOAA reported Kp=3+ this morning). We expect such a geomagnetic conditions to persist in the coming hours.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 059, gebaseerd op 16 stations.
Wolfgetal Catania | 082 |
10cm zonneflux | 136 |
AK Chambon La Forêt | 015 |
AK Wingst | 014 |
Geschatte Ap | 013 |
Geschat internationaal zonnevlekkengetal | 069 - Gebaseerd op 25 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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