Titlebook: Speeksel en speekselklieren; Betekenis voor de mo E.C.I. Veerman,A. Vissink Book 2014Latest edition Bohn Stafleu van Loghum 2014 moleculair

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E.C.I. Veerman,A.J.M. Ligtenbergof the Sun or the Galactic magnetic ?eld. As these background ?elds are usually nearly constant in time and space, they can be approximated by a homogeneous ?eld. If there are no additional ?elds, the particle trajectory is a perfect helix along which the par- cle moves at a constant speed. In reali

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E.C.I. Veerman,A. van Nieuw Amerongenof the Sun or the Galactic magnetic ?eld. As these background ?elds are usually nearly constant in time and space, they can be approximated by a homogeneous ?eld. If there are no additional ?elds, the particle trajectory is a perfect helix along which the par- cle moves at a constant speed. In reali

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H.S. Brand,E.C.I. Veermanighted. This knowledge is available in terms of probability density functions, and the nonlinearity means that the shape of these functions is unknown a-priori. We focus on sampling methods because of they flexibility. Traditional Monte-Carlo methods like Metropolis-Hastings and its variants are dis

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E.C.I. Veerman,W. van ’t Hof geometry, the deformation gradients will be introduced in the local curvilinear coordinate system, and the Green and Cauchy strain tensors will be presented. The length and angle changes will be discussed through Green and Cauchy strain tensors. The velocity gradient will be introduced for discussi