dc.contributor.author |
Camenen, Y |
en |
dc.contributor.author |
Peeters, AG |
en |
dc.contributor.author |
Angioni, C |
en |
dc.contributor.author |
Casson, FJ |
en |
dc.contributor.author |
Hornsby, WA |
en |
dc.contributor.author |
Snodin, AP |
en |
dc.contributor.author |
Strintzi, D |
en |
dc.date.accessioned |
2014-03-01T01:32:13Z |
|
dc.date.available |
2014-03-01T01:32:13Z |
|
dc.date.issued |
2009 |
en |
dc.identifier.issn |
0031-9007 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/20089 |
|
dc.subject |
Symmetry Breaking |
en |
dc.subject.classification |
Physics, Multidisciplinary |
en |
dc.subject.other |
Background flows |
en |
dc.subject.other |
Flux surfaces |
en |
dc.subject.other |
Magnetic configurations |
en |
dc.subject.other |
Magnetic field lines |
en |
dc.subject.other |
Physical systems |
en |
dc.subject.other |
Plasma currents |
en |
dc.subject.other |
Radial fluxes |
en |
dc.subject.other |
Symmetry-breaking |
en |
dc.subject.other |
Toroidal currents |
en |
dc.subject.other |
Toroidal magnetic fields |
en |
dc.subject.other |
Toroidal plasmas |
en |
dc.subject.other |
Toroidal rotations |
en |
dc.subject.other |
Turbulent momentums |
en |
dc.subject.other |
Plasma simulation |
en |
dc.subject.other |
Rotation |
en |
dc.subject.other |
Magnetic fields |
en |
dc.title |
Transport of parallel momentum induced by current-symmetry breaking in toroidal plasmas |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevLett.102.125001 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevLett.102.125001 |
en |
heal.identifier.secondary |
125001 |
en |
heal.language |
English |
en |
heal.publicationDate |
2009 |
en |
heal.abstract |
The symmetry of a physical system strongly impacts on its properties. In toroidal plasmas, the symmetry along a magnetic field line usually constrains the radial flux of parallel momentum to zero in the absence of background flows. By breaking the up-down symmetry of the toroidal currents, this constraint can be relaxed. The parallel asymmetry in the magnetic configuration then leads to an incomplete cancellation of the turbulent momentum flux across a flux surface. The magnitude of the subsequent toroidal rotation increases with the up-down asymmetry and its sign depends on the direction of the toroidal magnetic field and plasma current. Such a mechanism offers new insights in the interpretation and control of the intrinsic toroidal rotation in present day experiments. © 2009 The American Physical Society. |
en |
heal.publisher |
AMER PHYSICAL SOC |
en |
heal.journalName |
Physical Review Letters |
en |
dc.identifier.doi |
10.1103/PhysRevLett.102.125001 |
en |
dc.identifier.isi |
ISI:000264632100034 |
en |
dc.identifier.volume |
102 |
en |
dc.identifier.issue |
12 |
en |