Reply to comment by Yermolaev and Lodkina on "Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections" by Owens (2018) in arXiv:2008.05160
Mathew Owens
TL;DR
This paper provides a detailed response to critiques of Owens's 2018 study on solar wind and heavy ion properties in interplanetary coronal mass ejections, clarifying previous findings and addressing concerns.
Contribution
It offers a clarification and defense of Owens's original analysis in light of the comments by Yermolaev and Lodkina.
Findings
Clarifies the original analysis of solar wind properties
Addresses specific critiques raised by Yermolaev and Lodkina
Reaffirms the validity of Owens's conclusions
Abstract
Here I reply to the comment by Yermolaev and Lodkina [arXiv:2008.05160] on "Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections" by Owens (2018).
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Ionosphere and magnetosphere dynamics