Titlebook: Applied Mathematics and Computational Mechanics for Smart Applications; Proceedings of AMMAI Lakhmi C. Jain,Margarita N. Favorskaya,Dmitry

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Astronomical and Geophysical Factors of the Perturbed Chandler Wobble of the Earth Pole The contribution of the astronomical and geophysical disturbances to the observed Earth pole oscillations is discussed based on the processing of IERS observations of the Earth pole motion, NCEP/NCAR geophysical data of the atmospheric circulation, and NASA/JPL angular momentum of the ocean. The di

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Pareto-effiziente Risikoteilungs considered. The moment equations are supplemented by the diffusion equation of a condensing gas. To solve the equations, the finite volume method is used. The Riemann problem is solved using the AUSM+ method.

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Conference proceedings 2021ospace Industry (AMMAI 2020), held from September 6 to September 13, 2020, at the Alushta Health and Educational Center (The Republic of Crimea). The book is dedicated to solving actual problems of applied mechanics using modern computer technology including smart paradigms. Physical and mathematica

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Hirsutism

Deskriptive Entscheidungstheorie bei Risikorge temperatures behind a shock wave without consideration of the radiation at a considered short timescale. General EOS for the mixture of protons, electrons, and radiation differs from an ideal gas low EOS for two components (protons and electrons) fully ionized hydrogen plasma.

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https://doi.org/10.1007/978-3-322-92089-8ries and contact boundaries of the integrational domain. In the work, the process of propagation of elastic waves in the considered geological environment studies simulates the distribution of stresses and also studies the stability of the ice island to destruction using the Mises criterion.

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A Godunov-Type Method for a Multi-temperature Plasma with Strong Shock Waves and a General Equation rge temperatures behind a shock wave without consideration of the radiation at a considered short timescale. General EOS for the mixture of protons, electrons, and radiation differs from an ideal gas low EOS for two components (protons and electrons) fully ionized hydrogen plasma.