Vortices in stratified protoplanetary disks : From baroclinic instability to vortex layers

Autor: Barge, P., Richard, S., Dizes, S. Le

Publikováno v: A&A 592, A136 (2016)

Large scale vortices could play a key role in the evolution of protoplanetary disks, particularly in the dead-zone where no turbulence associated with magnetic field is expected. Their possible formation by the subcritical baroclinic instability is a

Externí odkaz: http://arxiv.org/abs/1602.09063

Magnetic field induced by elliiptical instability in a rotating tidally distorded sphere

Autor: Gal, P. Le, Lacaze, L., Dizès, S. Le

Publikováno v: Journal of Physics: conference Series 14 (2005) 30-34

It is usually believed that the geo-dynamo of the Earth or more generally of other planets, is created by the convective fluid motions inside their molten cores. An alternative to this thermal or compositional convection can however be found in the i

Externí odkaz: http://arxiv.org/abs/physics/0511226

Magnetic field induced by elliptical instability in a rotating spheroid.

Autor: Lacaze, L., Herreman, W., Bars, M. Le, Dizès, S. Le, Gal, P. Le

Publikováno v: Geophysical & Astrophysical Fluid Dynamics; Aug-Oct2006, Vol. 100 Issue 4/5, p299-317, 19p, 3 Color Photographs, 2 Diagrams, 6 Graphs

TOCATTA: a dynamic transfer model of ¹⁴C from the atmosphere to soil-plant systems.

Autor: Dizès SL; Institut de Radioprotection et de Sûreté Nucléaire (IRSN), DEI, SECRE, LME, CEN Cadarache Bât. 159, 13015 Cadarache, France. severine.ledizes@irsn.fr, Maro D, Hébert D, Gonze MA, Aulagnier C

Publikováno v: Journal of environmental radioactivity [J Environ Radioact] 2012 Feb; Vol. 105, pp. 48-59. Date of Electronic Publication: 2011 Nov 16.