Large-scale dynamo produced by negative magnetic eddy diffusivities

5: Features of the axial dipole dynamo: (a) evolution of the time-averaged axial magnetic field as a function of the rotation frequency for the three configurations; (b)

Comparing our simple helical magnetic field models with the observations, we find the observational measurements are consistent with the presence of a quadrupolar magnetic field

When a number is to be multiplied by itself repeatedly,  the result is a power    of this number.

We also propose that a plausible solution for the colder regions of the disk is accretion that is not driven by turbulence, but by removal of angular momentum by the wind torque in

Suppose that given x > 49 and using Sieve I we have a way to compute the number of permitted k-tuples whose indices lie in [1, x]; then, we could prove the main theorem

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

Intuitively, wherever the gradient of a function u is small, the function will be Lipschitz, so we should not need any further information from the equation at those points in order

Therefore, the phase-space trajectories of the fast parallel motion are supported by mag- netic field lines for their space dependence, have constant magnetic moment and are such