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This paper reexamines a basic test case used for spherical shallow-water numerical models, and underscores the need for accurate, high resolution models of atmospheric and ocean dynamics. The Rossby–Haurwitz test case, first proposed A standard test set for numerical approximations to the shallow-water equations on the sphere, J. Comput. Phys. (1992)(More)
Raman and x-ray photoelectron spectroscopy study of ferroelectric switching in Pb(Nb,Zr,Ti)O3 thin films Optical properties of cobalt slanted columnar thin films passivated by atomic layer deposition Appl. Intrinsic evolutions of optical functions, band gap, and higher-energy electronic transitions in VO2 film near the metal-insulator transition region(More)
An optical study of fully strained ultrathin LaNiO 3 films is presented and compared with LDA + DMFT calculations. LaNiO 3 films were grown by pulsed laser deposition on LaAlO 3 and SrTiO 3 substrates which provide compressive and tensile strain, respectively. Optical conductivity data show a Drude peak with a spectral weight that is significantly reduced(More)
Introduction: Since January 2004, OMEGA/Mars Express data has revealed a diverse and complex Martian surface mineralogy [1]. The important findings, together with Thermal Emission Spectrometer (TES), Thermal Emission Imaging System (THEMIS), and in-situ observations from Mars Exploration Rovers, include but not limited to These results are improving our(More)
Introduction: The Martian poles are covered by large quantities of water ice. The water ice in the north polar region is partially covered by CO 2 ice during the Martian winter and spring, and uncovered during the Martian summer and early fall, while in the south pole, the majority of water ice is normally covered by a thin bright CO 2 veneer [1,2,3,4].(More)
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