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Understanding particle drifts in a non-symmetric magnetic field is of primary interest in designing optimized stellarators to minimize the neoclassical radial loss of particles. Quasisymmetry and omnigeneity, two distinct properties proposed to ensur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98d2bd763ebc1e75924d5dfccf6b933b
