The Inversion of the Real Kinematic Properties of Coronal Mass Ejections by Forward Modeling
Y. Wu, P. F. Chen

TL;DR
This study uses forward modeling and Monte Carlo simulations to correct projection effects in CME observations, revealing that true velocities are higher and angular widths are smaller than observed values.
Contribution
It introduces a forward modeling approach to accurately estimate the real kinematic properties of CMEs, addressing biases in previous correction methods.
Findings
Real velocities of CMEs are approximately 514 km/s, higher than observed.
Real angular widths are about 33°, smaller than apparent measurements.
Corrected distributions improve understanding of CME dynamics.
Abstract
The kinematic properties of coronal mass ejections (CMEs) suffer from the projection effects, and it is expected that the real velocity should be larger and the real angular width should be smaller than the apparent values. Several attempts have been tried to correct the projection effects, which however led to a too large average velocity probably due to the biased choice of the CME events. In order to estimate the overall influence of the projection effects on the kinematic properties of the CMEs, we perform a forward modeling of the real distributions of the CME properties, such as the velocity, the angular width, and the latitude, by requiring their projected distributions to best match the observations. Such a matching is conducted by Monte Carlo simulations. According to the derived real distributions, it is found that (1) the average real velocity of all non-full-halo CMEs is…
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