Improved methods for determining the kinematics of coronal mass ejections and coronal waves
J. P. Byrne, D. M. Long, P. T. Gallagher, D. S. Bloomfield, S. A., Maloney, R. T. J. McAteer, H. Morgan, S. R. Habbal

TL;DR
This paper introduces improved, statistically rigorous methods for determining the kinematics of coronal mass ejections and coronal waves, emphasizing the use of the Savitzky-Golay filter and bootstrap techniques for more accurate and reliable estimates.
Contribution
It presents novel application of the Savitzky-Golay filter and bootstrap resampling to enhance the accuracy and robustness of CME and coronal wave kinematic measurements.
Findings
Savitzky-Golay filter improves fitting accuracy for CME kinematics
Bootstrap methods provide reliable error estimates and goodness-of-fit assessments
Enhanced measurement precision and sampling improve kinematic determination
Abstract
The study of solar eruptive events and associated phenomena is of great importance in the context of solar and heliophysics. Coronal mass ejections (CMEs) and coronal waves are energetic manifestations of the restructuring of the solar magnetic field and mass motion of the plasma. Characterising this motion is vital for deriving the dynamics of these events and thus understanding the physics driving their initiation and propagation. The development and use of appropriate methods for measuring event kinematics is therefore imperative. Traditional approaches to the study of CME and coronal wave kinematics do not return wholly accurate nor robust estimates of the true event kinematics and associated uncertainties. We highlight the drawbacks of these approaches, and demonstrate improved methods for accurate and reliable determination of the kinematics. The Savitzky-Golay filter is…
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