Introduction
The prediction of auroras (especially for Germany) is a complex matter that depends on many factors. Beginners in this field often find it difficult to understand and comprehend the physical processes. Therefore, we have attempted to explain the path from the creation of a coronal mass ejection to the aurora in individual stages.
- Interplanetary Magnetic Field
- Sunspots
- Flares
- Coronal Holes
- Arrival of the CME
- Geomagnetic storm
- Observe aurora
Further Information
- Collection on Aurora Forecast
- Detailed Tutorial on Auroras in Germany (Lutz Schenk, unfortunately never completed)