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To examine this scenario in detail, we performed μSR experiments as a function of longitudinal magnetic field (LF).
The most time-efficient way of beam vacuum optimization is using a 1D diffusion model where all parameters are defined as a function of longitudinal coordinate (along the beam path).
It was shown using shear-lag theory that for an exfoliated monolayer graphene flake deformed on a polymer substrate the strain in the graphene should be zero near the edges and increase toward the center of the flake such that 2where 3and where εm is the matrix strain and εr is the real strain of graphene as a function of longitudinal position x along the stress direction.
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The transient forces acting on them are a function of the longitudinal and transverse spacings and of the relative velocity between the two vehicles.
According to the results of numerical simulation, the tension of the cable is related to the cable length, which in turn is a function of the longitudinal and transverse displacements of the cable.
These are plotted as a function of the longitudinal co-ordinates along the duct for several values of the three dimensionless parameters in the problem, viz., (1) the relative height of wall corrugations, (2) the Mach number of the mean flow at the central section and (3) the wavenumber made dimensionless multiplying by the periodicity of corrugations.
A hypothesis is proposed that vertex points move affinely in the large-deformation regime, when the struts buckle, and that the force carried by a strut is a function of the longitudinal and rotational change of its vertex-to-vertex vector.
First, shear resistance relationship which expresses the shear degradation as a function of the longitudinal strain in the bottom reinforcement, among other variables.
Second, shear demand relationship which represents the required shear as the applied load increases, and also can be expressed as a function of the longitudinal strain in the bottom reinforcement.
Lario et al. (2006, 2013) were able to fit a Gaussian to the ensemble of multispacecraft SEP peak intensities as a function of the longitudinal distance between the solar source (inferred from flare observations) and the magnetic connection point for each spacecraft on the Sun.
The electron mobility as a function of the longitudinal electric field in the 2-DEG channel, μ n (E), is assumed to follow the Caughey and Thomas model given by[23] μ n E = μ n 0 1 + μ n 0 E v sat − 1 / β n cm 2 / V ‒ s (4).
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com