Superconductivity in ultra-thin CoSi2 epitaxial films

Hg^/H (T) has a minimum as a function of a/X(T) at about 1.12H C at a radius a = 3.8X(T) for K-values less than 0.16 \\ = GL penetration depth]- It is found that the

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

Finite thickness and loss of translational symmetry along the surface normal result in magnetic size ef- fects, like reduction of J, and T, [I, 21, and in inho-

Further studies concerning the magnetic p r o p erties of these films are in progress, in particular the investigation of the thermomagnetic writing process

We have studied the propagation of highest energy cosmic rays in the Galactic magnetic field, for different assumptions on the large-scale field structure and/or primary cosmic ray

Critical currents in superconducting networks and magnetic field

In other cases the Curie temperature is smaller than the crystallisation temperature and the annealing up to the Curie temperature induces a more rapidly decrease of p, with

2014 The classical Lorentz field in a spherical cavity of 403C0 Ms/3 does not occur in a ferromagnetic material which has reached technical saturation.. This effect