Datum verslag: 2019 Sep 26 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
26 Sep 2019 | 068 | 007 |
27 Sep 2019 | 068 | 010 |
28 Sep 2019 | 068 | 031 |
Solar X-ray flux remained below B class levels throughout the period. The Solar disk is spotless and the X-ray flux is expected to remain at or below background levels.
There were no Earth-directed Coronal Mass Ejections (CME) observed in coronagraph data.
Proton levels were at background values and are expected to remain so.
The solar wind speed has decreased from 440 and 400 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 4 nT. The Bz ranged between -5 and 3 nT, but was mainly positive. Geomagnetic conditions ranged between Kp index 1-3 (NOAA) and local K index 1-3 (Dourbes).
The solar wind conditions declined over the past 24 hours as we moved into background solar wind conditions following the passing of a high speed stream (HSS), from a small recurrent equatorial coronal hole.
Tomorrow and the next day we expect solar wind conditions to become enhanced due to the presence of a second larger recurrent coronal hole, which passed the central meridian yesterday. On the coronal holes last rotation the resultant HSS produced minor storm conditions for short periods.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 000, gebaseerd op 13 stations.
Wolfgetal Catania | 000 |
10cm zonneflux | 068 |
AK Chambon La Forêt | 010 |
AK Wingst | 004 |
Geschatte Ap | 003 |
Geschat internationaal zonnevlekkengetal | 000 - 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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