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Scaling law: Difference between revisions
→Confinement time scaling
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For [[stellarator]]s, a similar scaling has been obtained (ISS). | For [[stellarator]]s, a similar scaling has been obtained (ISS). | ||
<ref>[http://www.ipp.mpg.de/ISS ISS-IPP] and [http://iscdb.nifs.ac.jp/ ISS-NIFS] homepages</ref> | <ref>[http://www.ipp.mpg.de/ISS ISS-IPP] and [http://iscdb.nifs.ac.jp/ ISS-NIFS] homepages</ref> | ||
<ref> | <ref>A. Dinklage et al, ''Physical model assessment of the energy confinement time scaling in stellarators'', [[doi:10.1088/0029-5515/47/9/025|Nucl. Fusion '''47''', 9 (2007) 1265-1273]]</ref> | ||
* ISS04v3 | * ISS04v3 | ||
:<math>\tau_E = 0.148 R^{0.64} a^{2.33} \bar n_{20}^{0.55} B^{0.85} \iota_{2/3}^{0.41} P^{-0.61}</math> | :<math>\tau_E = 0.148 R^{0.64} a^{2.33} \bar n_{20}^{0.55} B^{0.85} \iota_{2/3}^{0.41} P^{-0.61}</math> | ||