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Sudo limit: Difference between revisions
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:<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 == | == See also == | ||