Forward modeling of coronal mass ejection flux ropes in the inner heliosphere with 3DCORE

2 Oct 2017Christian MöstlTanja AmerstorferErika PalmerioAlexey IsavninCharles J. FarrugiaChris LowderReka M. WinslowJulia DonnererEmilia K. J. KilpuaPeter D. Boakes

Forecasting the geomagnetic effects of solar storms, known as coronal mass ejections (CMEs), is currently severely limited by our inability to predict the magnetic field configuration in the CME magnetic core and by observational effects of a single spacecraft trajectory through its 3D structure. CME magnetic flux ropes can lead to continuous forcing of the energy input to the Earth's magnetosphere by strong and steady southward-pointing magnetic fields... (read more)

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