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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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Modeling the Degradation of Small Lunar Impact Craters: an Example Using a DEM (Digital Elevation Model)

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Modeling the Earth's magnetospheric magnetic field confined within a realistic magnetopause

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Modeling the Non-linear Viscoelastic Response of High Temperature Polyimides

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Modeling whistler wave generation regimes in magnetospheric cyclotron maser

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Modelling of the effect of current-carrying jets on the temperature of an astrophysical surrounding

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Modelling rotation curves -- the turbulent way

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Models of angular momentum input to a circum-terrestrial swarm from encounters with heliocentric planetesimals

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Models of the convective envelope of B-F stars

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Models of the cosmological evolution of extragalactic radio sources. I - The 408-MHz source count

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Modern Statistics by Kriging

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Modification of the nebular environment in symbiotic systems due to colliding winds

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Molecule formation and destruction processes in astrophysical environments

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Moment-ration imaging of seismic regions for earthquake prediction

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Motion of artificial satellites in the set of Eulerian redundant parameters. III

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Multi-ion resonances in finite temperature plasma

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Multi-objective Geometric Programming Problem With Weighted Mean Method

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