| Subject |
Curriculum |
Semester |
Credit |
| 1 |
2 |
3 |
4 |
| Thermodynamics and statistical physics |
|
4 |
|
|
|
4 |
| Thermodynamics and statistical physics |
|
1 |
|
|
|
2 |
| Nuclear physics |
|
|
2 |
|
|
2 |
| Astrophysics |
|
2 |
|
|
|
2 |
| Astrophysics |
1. Stationary radiative transfer in stellar atmospheres. (Basic quantities and laws of radiation theory, their connection with observed spectroscopic quantities. Monochromatic transfer equation and its solution. Grey atmospheres. Radiative equilibrium.
2. Equilibrium of a stellar atmosphere. (Local thermodynamic equilibrium - LTE - and NLTE. Hydrostatic equilibrium. Convection in stellar atmospheres. Simplified and constant flux model atmospheres.)
3. Brief theory of line formation in stellar atmospheres. (Oscillator strength, their calculation in quantum mechanics. Line broadening.)
4. Evaluation of astronomical spectra. (Determination of physical parameters of stars. Curve of growth, fine analyse by line profils. Cosmic abundances from stellar spectra. Baade-Wesselink method. Spectra of galaxies and quasars.) |
|
2 |
|
|
2 |
| Astrophysics |
Stellar (Magneto) Hydrodynamics (Dynamical Principles, Conservation of Energy, Circulation and Vorticity, Stellar Hydromagnetics); Nuclear Energy Production; Transport of Energy (by radiation, conduction and convection); Stellar Models: Techniques; Simple Stellar Models (Polytropic Gaseous Spheres); Stellar Evolution (Star formation, Main Sequence, Massive Stars, Low-mass Stars, Latter Phases); Pulsating Stars; Stellar Oscillations |
|
|
2 |
|
2 |
| Astrophysics |
The solar interior; Solar rotation; Observing tools of solar physics; The quiet photosphere; Chromosphere and corona; Solar activity; Elements of dynamo theory;The solar wind and the heliosphere |
|
|
|
2 |
2 |
| Astrophysics maturandum |
|
|
|
X |
|
3 |
| Celestial mechanics |
Theory of motion of Earth's artificial satellites
(Representation of the Earth's gravitational potential by spherical harmonics. Kaula's expansion of the perturbing function. The main gravitational perturbations caused by Earth. Theory of intermediate orbits. Critical inclination. Synchronous satellites. Luni-solar perturbations. Non-gravitational perturbations.) |
2 |
|
|
|
2 |
| Celestial mechanics |
Dynamics of the Solar System
(Canonical theories of perturbations: Hamilton-Jacobi method, Poincaré-Zeipel method, theory of secular perturbations, Lie-transformation method. The KAM-theorem. Methods of chaos detection. Chaotic phenomena in the Solar system and in exoplanetary systems.) |
|
2 |
|
|
2 |
| Celestial mechanics |
The three-body problem
(The general three-body problem: Sundman theorem, Lagrange-Jacobi equation, classification of final motions, the Euler-Lagrange solutions. The restricted three-body problem: synodical equations of motion, Jacobi integral, zero velocity curves, equilibrium solutions and their stability, regularization, periodic solutions, numerical investigations.) |
|
|
2 |
|
2 |
| Celestial mechanics |
Selected problems of celestial mechanics
(Resonances: the geometry of resonances, the first model of the resonance (the pendulum), the second fundamental model of resonances, resonant encounters, resonances in the restricted three-body problem, resonances in the Solar system and in exoplanetary systems. Symplectic mappings and their application in celestial mechanics.) |
|
|
|
2 |
2 |
| Celestial mechanics maturandum |
|
|
X |
|
|
3 |
| Galactic astronomy |
Basic features of the Milky Way, foundations of stellar statistics, stellar groups and associations, stellar kinematics and dynamics, rotation of the Galaxy. |
2 |
|
|
|
2 |
| Galactic astronomy |
Spiral structure, galactic halo, chemical composition and evolution of the Galaxy, central region of the Milky Way, galactic magnetic field and the galactic corona, galactic x-ray radiation, cosmic radiation. |
|
2 |
|
|
2 |
| Galactic astronomy |
Extragalactic distance measurement, morphology of galaxies, peculiar galaxies, spatial distribution of galaxies, photometric and spectral properties of galaxies. |
|
|
2 |
|
2 |
| Galactic astronomy |
Active galaxies, the unified model of active galaxy nuclei, gravitational lensing, cosmic microwave background radiation, primordial nucleosynthesis, formation of structures. |
|
|
|
2 |
2 |
| Galactic astronomy maturandum |
|
|
|
X |
|
3 |
| Cosmology |
Foundations of GR, model solutions of field-equations, proofs of the standard model, the early Universe, formation of structures, alternative cosmologies, observational cosmology. |
|
|
|
2 |
2 |
| Astronomical spectroscopy |
|
2 |
|
|
|
2 |
| Astronomical spectroscopy |
|
|
2 |
|
|
2 |
| Astonomical seminar |
|
2 |
|
|
|
2 |
| Astonomical seminar |
|
|
2 |
|
|
2 |
| Astonomical seminar |
|
|
|
2 |
|
2 |
| Astonomical seminar |
|
|
|
|
2 |
2 |
| Thesis seminar |
|
|
10 |
|
|
10 |
| Thesis seminar |
|
|
|
20 |
|
20 |
| Thesis seminar |
|
|
|
|
20 |
20 |
| Closing maturandum |
|
|
|
|
X |
|
