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Method for determining the velocity of the center of mass of a spacecraft on the basis of results of trajectory measurements

Computer Science – Numerical Analysis
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Methods of astrometry for minor planets. II - Mathematical evaluation

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MHD Modeling of the Interaction of the Solar Wind With Venus

Computer Science – Numerical Analysis
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MHD shocks in coronal mass ejections

Computer Science – Numerical Analysis
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MHD turbulent mixing layers

Computer Science – Numerical Analysis
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MHD vortex mechanism of cometary rays origin

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Microstructural changes as a result of temperature gradients in the Al-Al3Ni eutectic

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Microwave imaging of Mercury's thermal emission at wavelengths from 0.3 to 20.5 CM

Computer Science – Numerical Analysis
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Millstone Hill incoherent scatter F region observations during the disturbances of June 1991

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Minimum orbits about the planet Venus

Computer Science – Numerical Analysis
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Mirror deformations due to thermal expansion of inserts bonded to glass

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MO and DA on the SWIE Instrument on the Wind Spacecraft

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Modal fields: A new method for characterization of random seismic velocity heterogeneity

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Mode identification of pulsating stars from line profile variations with the moment method. A theoretical study of the accuracy of the method

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Model Checking CSL for Markov Population Models

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Model of diurnal variations of thermosphere parameters. II - Computational results

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Model stellar atmospheres. I - Numerical techniques

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Modeling of Gas Flow Structure in Symbiotic Star Z And in Quiescent and Active States

Computer Science – Numerical Analysis
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Modeling of transient disturbances in coronal-streamer configurations

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Modeling radio-wave scattering by a traveling spherical disturbance in the ionosphere

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