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Introduction to Space Gas-Dynamics

PROGRAM of

'Introduction to Space Gas-Dynamics'

Fifth Year


  • Introduction. General Ideas of Structure and Physical Parameters of Interstellar Medium. Chemical Structure of Interstellar Gas. Main Components of Interstellar Medium: Molecular Clouds, Diffuse Clouds HI, Intercloud Medium, HII Zone, Coronal Gas. Super-Clouds, Giant Molecular Clouds, Stellar Complexes, Super-Envelopes. Physical Processes, Which Have an Influence on Interstellar Medium State.
  • Basic Ideas of Gas-Dynamics. Basic Equations. Perfect Viscous, Heat-Conducting Liquid. Streams of Energy and Impulse. Hydrostatics.
  • Gas-Dynamics Stability. Conception of Stability. Perturbation Method.
  • Discontinuity Surfaces. Types of Discontinuities. Correlations on the Discontinuity Surfaces. Stationary Shock Waves. Shock Waves with Decay. Detonation Waves.
  • Nonstationary Shock Waves. Conception of Scaling. Approximation of Infinitely Thin Layer. Problem of Point Explosion. Shock Wave Propagation in Exponential Mediums. 'Break of the Atmosphere'.
  • Physical State of the Interstellar Medium Regulated by Active Processes. Supernovae. Brightness Curves, Spectrums, Types, Energy, Frequency of Bursts. Basic Evolution Stages. Interaction of Supernovae Remains with Interstellar Medium.
  • Stellar Wind. Interaction of Stellar Wind with Interstellar Gas. Ionization Fronts. Origin and Dynamics of Gigantic Envelopes of Neutral and Ionized Hydrogen.
  • Motion in Gravitation Field. Spherical and Disc Accretion. Stability of Infinitely Thin Gravitating Rotating Disc. The Nature of the Spiral Structure of Galaxies.

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