• Corpus ID: 221103864

Comment on "Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections" by M.J.Owens.

@article{YuIYermolaev2020CommentO,
  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: Space Physics},
  year={2020}
}
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. 

References

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The heliospheric counterparts of coronal mass ejections (CMEs) at the Sun, interplanetary coronal mass ejections (ICMEs), can be identified in situ based on a number of magnetic field, plasma,

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