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The SOLA method for helioseismic inversion

Computer Science – Numerical Analysis
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The solar atmosphere and the structure of active regions

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The solar corona as a quadric surface in three-dimensional space

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The solar wind termination shock in the presence of cosmic rays

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The Spiralling Binary System of Black Holes.

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The stability of 2D current sheet models of prominences

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The stability of perfect elliptic disks. 1: The maximum streaming case

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The stability of periodic motions of a satellite relative to its own center of mass

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The stability of spherically symmetric accretion flows

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The stellar content of the nuclei of late-type spiral galaxies

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The stellar dynamics of 'box/peanut' galactic bulges

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The Stochastic Logarithmic Norm for Stability Analysis of Stochastic Differential Equations

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The structure and evolution of 'asteroidal' meteor swarms

Computer Science – Numerical Analysis
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The study of planetary secular perturbations

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The study of the physics of cometary nuclei

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The subsonic structure of radiatively driven winds of early-type stars

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The supernova neutrino pulse shape in the scintillation detector

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The synthesis of light curves of close binary systems with a relativistic object - Axisymmetric geometrically thick disk around a relativistic object

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The telegraph equation in charged particle transport

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The temperature-density structure of coronal loops in hydrostatic equilibrium

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