Fast Method to Determine CMEs properties at 1 AU and Propositions for an Automated Detection of CME Fronts

Astronomy and Astrophysics – Astrophysics

Scientific paper

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[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7924] Space Weather / Forecasting

Scientific paper

Coronal mass ejections (CMEs), when directed towards Earth, are the primary driver for space weather. It is therefore important to predict their arrival time at Earth, as well as their speed and other characteristics. We propose a snow-plow analytical model that we apply to some CMEs using 3-D steady-state solar wind driven by magnetic field observations. The results are compared with other from existing methods and in situ observations, giving good estimation of CMEs arrival time to 1AU. We also present different image processing methods and preliminary results for automated detection of CMEs front and shape. These preliminary results are compared to data were the intervention of human judgment played a mayor role.

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