Sudo limit: Difference between revisions
Jump to navigation
Jump to search
(Created page with "The Sudo limit is an operational limit for the density in stellarators<ref>Sudo S. et al, ''Scalings of energy confinement and density limit in stellarator/heliotron devices'', Nucl. Fusion '''30''' (1990) 11</ref>: :<math>n_S \propto \sqrt{P_hB/V} </math> == References == <references/>") |
No edit summary |
||
| (One intermediate revision by the same user not shown) | |||
| Line 2: | Line 2: | ||
:<math>n_S \propto \sqrt{P_hB/V} </math> | :<math>n_S \propto \sqrt{P_hB/V} </math> | ||
Beyond this limit, radiative collapses are frequently observed<ref>G. Fuchert et al., ''Increasing the density in Wendelstein 7-X: benefits and limitations'', [[doi:10.1088/1741-4326/ab6d40|Nucl. Fusion '''60''' (2020) 036020]]</ref>. | |||
== See also == | |||
[[Greenwald limit]] | |||
== References == | == References == | ||
<references/> | <references/> | ||
Latest revision as of 06:30, 23 October 2024
The Sudo limit is an operational limit for the density in stellarators[1]:
Beyond this limit, radiative collapses are frequently observed[2].
See also
References
- ↑ Sudo S. et al, Scalings of energy confinement and density limit in stellarator/heliotron devices, Nucl. Fusion 30 (1990) 11
- ↑ G. Fuchert et al., Increasing the density in Wendelstein 7-X: benefits and limitations, Nucl. Fusion 60 (2020) 036020