Profile consistency: Difference between revisions

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Profile consistency (or profile resilience) is the observation that profiles (of temperature, density, and pressure) often tend to adopt roughly the same shape (in tokamaks), regardless of the applied heating and fueling profiles.
Profile consistency (or profile resilience) is the observation that profiles (of temperature, density, and pressure) often tend to adopt roughly the same shape (in [[Tokamak|tokamaks]]), regardless of the applied heating and fueling profiles.
<ref>B. Coppi, ''Nonclassical Transport and the "Principle of Profile Consistency"'', Comments Plasma Phys. Cont. Fusion '''5''', 6 (1980) 261-270</ref>
<ref>B. Coppi, ''Nonclassical Transport and the "Principle of Profile Consistency"'', Comments Plasma Phys. Cont. Fusion '''5''', 6 (1980) 261-270</ref>
<ref>Yu.N. Dnestrovsky et al, Sov. J. Plasma Phys. '''16''' (1990) 120</ref>
<ref>Yu.N. Dnestrovsky et al, Sov. J. Plasma Phys. '''16''' (1990) 120</ref>
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i.e., the feedback mechanism regulating the profiles (by turbulence) is often dominant over the various source terms.
i.e., the feedback mechanism regulating the profiles (by turbulence) is often dominant over the various source terms.
<ref>[http://link.aip.org/link/?PHPAEN/8/4096/1 F. Jenko et al, ''Critical gradient formula for toroidal electron temperature gradient modes'', Phys. Plasmas '''8''' (2001) 4096]</ref>
<ref>[http://link.aip.org/link/?PHPAEN/8/4096/1 F. Jenko et al, ''Critical gradient formula for toroidal electron temperature gradient modes'', Phys. Plasmas '''8''' (2001) 4096]</ref>
Recently, some indication of profile consistency has also been obtained for [[Stellarator|stellarators]].
<ref>[http://www-pub.iaea.org/MTCD/Meetings/FEC2008/th_p8-24.pdf Yu.N. Dnestrovsky et al, IAEA Fusion Energy Conference, Geneva (2008) TH/P8-24]</ref>


== References ==
== References ==
<references />
<references />

Revision as of 09:24, 20 September 2010

Profile consistency (or profile resilience) is the observation that profiles (of temperature, density, and pressure) often tend to adopt roughly the same shape (in tokamaks), regardless of the applied heating and fueling profiles. [1] [2] The resulting (stiff) profiles are known as canonical profiles. [3] This phenomenology is due to plasma self-organisation, [4] i.e., the feedback mechanism regulating the profiles (by turbulence) is often dominant over the various source terms. [5]

Recently, some indication of profile consistency has also been obtained for stellarators. [6]

References