Morphology of two-dimensional MRI in axial symmetry

@article{50440,
   author = {Pugliese, Daniela and Montani, },
   article_location = {US - Spojené státy americké},
   article_number = {6},
   doi = {http://dx.doi.org/10.1017/S0022377815001142},
   keywords = {accretion disks; magneto-hydrodynamics; plasma phenomena},
   language = {eng},
   issn = {0022-3778},
   journal = {Journal of Plasma Physics},
   title = {Morphology of two-dimensional MRI in axial symmetry},
   url = {https://www.cambridge.org/core/journals/journal-of-plasma-physics/article/abs/morphology-of-twodimensional-mri-in-axial-symmetry/A3F7AD9C7AD013066F4A475D7C52D6A1},
   volume = {81},
   year = {2015}
}

TY  - JOUR
ID  - 50440
AU  - Pugliese, Daniela - Montani,
PY  - 2015
TI  - Morphology of two-dimensional MRI in axial symmetry
JF  - Journal of Plasma Physics
VL  - 81
IS  - 6
SP  - "495810604-1"-"495810604-9"
EP  - "495810604-1"-"495810604-9"
SN  - 00223778
KW  - accretion disks
KW  - magneto-hydrodynamics
KW  - plasma phenomena
UR  - https://www.cambridge.org/core/journals/journal-of-plasma-physics/article/abs/morphology-of-twodimensional-mri-in-axial-symmetry/A3F7AD9C7AD013066F4A475D7C52D6A1
N2  - In this paper, we analyse the linear stability of a stellar accretion disk having a stratified morphology. The study is performed in the framework of ideal magneto-hydrodynamics and therefore results in a characterization of the linear unstable magneto-rotational modes. The peculiarity of the present scenario consists of adopting the magnetic flux function as the basic dynamical variable. Such a representation of the dynamics allows us to take account of the co-rotation theorem as a fundamental featureof the ideal plasma equilibrium and to evaluate its impact on the perturbation evolution. According to the Alfvenic nature of the magneto-rotational instability, we consider an incompressible plasma profile and perturbations propagating along the background magnetic field. Furthermore, we develop a local perturbation analysis around fiducial coordinates of the background configuration and deal with very small-scale linear dynamics in comparison to the background inhomogeneity size. The m
ER  - 

PUGLIESE, Daniela a MONTANI. Morphology of two-dimensional MRI in axial symmetry. \textit{Journal of Plasma Physics}. US - Spojené státy americké, 2015, roč.~81, č.~6, s.~''495810604-1''-''495810604-9'', 9 s. ISSN~0022-3778. Dostupné z: https://dx.doi.org/10.1017/S0022377815001142.