Time-consistent estimators of 2D/3D motion of atmospheric layers from pressure images

The main goal of this paper is to provide another solution for the problem of the motion of stars in galaxies by using a new gravitational time dilation for the weak gravitational

The unitary maps ϕ 12 will be very useful in the study of the diagonal action of U(2) on triples of Lagrangian subspaces of C 2 (see section 3).. 2.4

Horizontal winds estimated with the 3D-ICE model are superimposed on cloud pressure difference images for the high (left), the medium (middle) and the low (right) layer and

The 3D motion analyzer (Shimano Dynamics Lab, Sittard, Netherland) is a new kinematic system positioned in the sagittal plane and tracking LED markers attached to

Then the data term of the optical flow formulation is based on a stochastic transport equation, derived from a location uncertainty principle [17].. In addition, a

The joint continuity as well as Hölder conditions in both the space and the (time) set variable of the local time of locally nondeterministic (LND) Gaussian process and fields have

The position stabilization (pink background) is performed with a diode laser at λ = 980 nm, whose reexion from the wire top facet is detected on a quadrant photodiode (QPD) feeding

The following results are obtained: (1) the exact solution describing the stationary thermocapillary con- vective flow is found; (2) a priori estimates of the initial boundary