Direct construction of optimized stellarator shapes. Part 3. Omnigenity near the magnetic axis – ERRATUM.

Bibliographic Details
Title:	Direct construction of optimized stellarator shapes. Part 3. Omnigenity near the magnetic axis – ERRATUM.
Authors:	Plunk, Gabriel G.¹ (AUTHOR) gplunk@ipp.mpg.de, Landreman, Matt² (AUTHOR), Helander, Per¹ (AUTHOR)
Source:	Journal of Plasma Physics. Dec2021, Vol. 87 Issue 6, p1-2. 2p.
Subject Terms:	MAGNETIC flux density, TOROIDAL plasma
Abstract:	Our definitions for $d$ Graph and $\epsilon$ Graph affect the forms of the first order components of the coordinate mapping, $X 1$ Graph and $Y 1$ Graph. Our forms of $B$ Graph, $X 1$ Graph and $Y 1$ Graph can be compared with (79)-(81) of Garren & Boozer (1991), and can be seen to agree, given our definitions of $\epsilon$ Graph, $d$ Graph and $\bar {d}$ Graph, and the substitution $\kappa \rightarrow \kappa ^s$ Graph. \end{equation} Graph Note the factor of $\epsilon$ Graph is missing in the paper. [Extracted from the article]
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