Dislocation core field. I. Modeling in anisotropic linear elasticity theory

Mercury core dynamo field has its magnetic north pole located near the geographic

Le théo- rème 1 de [5] est notre présent théorème 1, le théorème 2 de [5] est notre théo- rème 2 réduit aux nombres premiers usuels, et le théorème 3 de [5] est notre

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

glissile core that governs the mobility of dislocations, In the instance of beryllium deformed in prismatic slip (figure 1), a substantial temperature shift between

Using a Keating potential, Jones [7] showed the formation energy of a single kink on a reconstructed 90° dislocation was about 0.5 eV and its migration energy was 2.7 eV.. There is

A sensitivity comparison using generic dense city parameters, derived from the Coordination of Information on the Environment (CORINE) land cover database, and those from a

In the case of an Alfv´ en wave turbulence (many wave packets) in a spherical shell of radius L with homogeneous mean energy e, permeated by a magnetic field of rms intensity B 0 ,

Truss and nucleus decomposition. In a more recent work, Sariy¨ uce et al. [129] capitalized on the relationship between core number and h-index [98], in order to propose efficient