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The role of gravitational potential energy in the Martian lithospheric stress field

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The Role of Hall Electric Fields in Two-dimensional Forced Magnetic Reconnection

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The role of initial binaries in cluster evolution - Direct N-body calculations

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The role of merged interaction regions and drafts in the heliospheric modulation of cosmic rays beyond 20 AU - A computer simulation

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The role of secondary resonances in the orbital history of Miranda

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The role of sound waves in Be-star winds

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The role of the dwarf nova period distribution in understanding the evolution of cataclysmic variables

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The role of the equation of state in the 'prompt' phase of type II supernovae

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The role of the tachocline for the solar dynamo

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The Role of Theoretical Atomic Physics in Astrophysical Plasma Modeling

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The role of turbulent convection in the primitive solar nebula II. Results

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The Roles and Needs of Models in the Future Solar-Terrestrial Data Environment

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The Rosseland mean free-free Gaunt factor of the dense high-temperature stellar plasma

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The Rosseland mean opacity of interstellar grain

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The rotation curve in the outer region of the Galaxy

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The rotation curve of NGC 3115

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The rotation curve of the Milky Way to 2.5 R0 from the thickness of the H I layer

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The rotation effect - A mechanism for measuring granulation velocities in stars

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The rotation of the solar atmosphere at different altitudes

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The rotation period, direction of the north pole, and geodetic control network of Venus

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