The effect of tangential drifts on neoclassical transport in stellarators close to omnigeneity
In general, the orbit-averaged radial magnetic drift of trapped particles in stellarators is non-zero due to the three-dimensional nature of the magnetic field. Stellarators in which the orbit-averaged radial magnetic drift vanishes are called omnigeneous, and they exhibit neoclassical transport lev...
Egile Nagusiak: | Calvo, I, Parra Diaz, F, Velasco, J, Alonso, J |
---|---|
Formatua: | Journal article |
Argitaratua: |
IOP Publishing
2017
|
Antzeko izenburuak
-
Less constrained omnigeneous stellarators
nork: Parra, F, et al.
Argitaratua: (2014) -
When omnigeneity fails
nork: Parra, F, et al.
Argitaratua: (2014) -
Stellarators close to quasisymmetry
nork: Calvo, I, et al.
Argitaratua: (2013) -
Flow damping in stellarators close to quasisymmetry
nork: Calvo, I, et al.
Argitaratua: (2014) -
Large tangential electric fields in plasmas close to temperature screening
nork: Velasco, J, et al.
Argitaratua: (2018)