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A novel X-ray diffraction technique with almost complete insensitivity to sample morphology

Statistics – Applications
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A nuclear spectroscopic survey of disk galaxies. II - Galaxies with emission lines not excited by stellar photoionization

Statistics – Methodology
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A Nuclear-Powered Laser-Accelerated Plasma Propulsion System

Statistics – Applications
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A numerical algorithm for geophysical and astrophysical inhomogeneous fluid flows

Statistics – Computation
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A Numerical Algorithm for Modeling Neutrino-Radiation Hydrodynamics in Two Spatial Dimensions

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A numerical analysis of seismic waves for an anisotropic fault zone

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A numerical analysis of transient planetary waves and the vertical structure in a meso-strato-troposphere model, part 1.4A

Statistics – Computation
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A Numerical Approach to Performance Analysis of Quickest Change-Point Detection Procedures

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A numerical hydrodynamic model of a heated coronal loop

Statistics – Computation
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A numerical implementation of MHD in divergence form

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A numerical investigation of the Kelvin-Helmholtz instability in the context of accreting neutron stars

Statistics – Computation
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A numerical method based on the Fourier-Fourier transform approach for modeling 1-D electron plasma evolution

Statistics – Computation
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A Numerical Method for Solving Systems of Linear Ordinary Differential Equations with Rapidly Oscillating Solutions

Statistics – Computation
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A numerical method for solving the neutrino Boltzmann equation coupled to spherically symmetric stellar core collapse

Statistics – Computation
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A numerical method to determine the electromagnetic field of the pulsar magnetosphere with inclined magnetic moment

Statistics – Computation
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A numerical model for an alternative origin of Lake Vostok and its exobiological implications for Mars

Statistics – Computation
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A numerical model of cohesion in planetary rings

Statistics – Applications
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A numerical model of the ionospheric signatures of time-varying magneticreconnection: I. ionospheric convection

Statistics – Applications
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A Numerical Package for Modeling Solar Flares and Interpreting HESSI Data

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A numerical scheme improving Hartle's perturbative method for treating general relativistic rotating neutron stars

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