Datum verslag: 2020 Aug 10 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 10 Aug 2020 | 073 | 005 |
| 11 Aug 2020 | 072 | 007 |
| 12 Aug 2020 | 072 | 007 |
The solar activity was quiet over the past 24 hours. The bipolar sunspot (NOAA-AR 2770) has slightly declined and did not produce any significant flaring activity. The X-ray flux remained below B-class level. The solar activity is expected to remain at low levels with a low probability of occurring a C-class flare.
No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery in the last 24 hours.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to stay at nominal levels for the next 24 hours. The greater than 2 MeV electron flux reached high levels over the past 24 hours and is expected to remain at high levels over the next 24 hours.
The Earth is currently under the influence of the slow solar wind streams. The solar wind parameters (DSCOVR) show at nominal values with the solar wind speed around 310-400 km/s, the total interplanetary magnetic field below 6 nT, and the Bz magnetic field components fluctuating between -3 nT and +5 nT. The solar wind conditions are expected to remain mostly nominal for the next days. A relatively small equatorial coronal hole (negative polarity) is currently facing Earth. The wind streams associated with this coronal hole may enhance the solar wind parameters near Earth in about 3-4 days for now.
Geomagnetic conditions were quiet, and quiet conditions are expected for the next following day.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 012, gebaseerd op 25 stations.
| Wolfgetal Catania | /// |
| 10cm zonneflux | 074 |
| AK Chambon La Forêt | 005 |
| AK Wingst | 002 |
| Geschatte Ap | 002 |
| Geschat internationaal zonnevlekkengetal | 012 - Gebaseerd op 34 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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