A recent paper by Owens (2018) presents a statistical analysis of the properties of interplanetary coronal mass ejections (ICMEs) and variations in their compositions and ion charge-state signatures using data from the Advanced Composition Explorer (ACE) spacecraft. However, the article contains several serious flaws, which we will discuss here.
@article{arxiv.2008.05160,
title = {Comment on "Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections" by M.J.Owens},
author = {Yu. I. Yermolaev and I. G. Lodkina},
journal= {arXiv preprint arXiv:2008.05160},
year = {2020}
}