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Application of the Three-Body Problem in the form of exercises
Kolář, Karel ; Šolc, Martin (advisor) ; Franc, Tomáš (referee)
The main topic of this work is the Restricted Three-Body Problem (R3BP) which is illustrated by solving several examples and by simulations in computational system Wolfram Mathematica. The aim is to offer supplemetary material for university students and it can be used also as introduction to this topic for high school students. The first part is dedidated to history of celestial mechanics and to the people who contributed to the development of the R3B Problem. The second chapter consists of simplier tasks with definitions of basic quantities and variables and revision of the undisturbed two-body problem. Subsequent chapters are concentrated to Lagrange points, Jacobi integral, Hill surfaces, tidal force, Tisserand criterion, shape and evolution of close binary stars and other partial tasks.
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Shell galaxies - "sticky particles" hydrodynamical simulations
Zimandl, Martin ; Jungwiert, Bruno (advisor) ; Šolc, Martin (referee)
Shell galaxies are usually ellipticals with concentric faint arc-like stellar structures with sharp outer edges. They originate from galactic collisions (so called mergers). According to observations, some galaxies has also gaseous structures, that can be associated with stellar shells. We carry out a few numerical simulations, in which we recreate gaseous shells throug radial collisions of small and large elliptical galaxies. Then we analyze the differences between stellar and gaseous shells. Our simulations are based on earlier models, which describes gas by using so called "sticky-particles" hydrodynamics. This approach was so far quite succesful in resolving origin of gaseous shells. Our conclusion is, that gas in preset galaxies is not sufficient to make any difference. Higher quantities on the other hand has significant effect. Powered by TCPDF (www.tcpdf.org)
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Forbidden Oxygen line emission from the traces of meteors
Habuda, Pavol ; Borovička, Jiří (advisor) ; Šolc, Martin (referee)
The aim of this diploma thesis was to study forbidden green oxygen line emission. It was found out that green line emit mainly in heights 100-110 kilometers, exceptionally below 90 kilometers. Time evolution of green line intensity with respect of heights was investigated in detail. There was suggested theoretical dependency and agreement with observed data was fulfilled. Dependency of integral intensity was investigated as well. Mechanisms of excitation and quenching of green line in emission was proposed in previous studies in 70. of previous century. This work discuss with its results. Efficiency of transformation of kinetic energy of meteoroid to forbidden green line's emission was discussed. The concentrations of atomic oxygen was estimated by several way in heights of green line emission.
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Simulation of the astrolabe of the Prague astronomical clock for PC
Makara, Tomáš ; Šolc, Martin (advisor) ; Brož, Miroslav (referee)
In this work we create a computer simulation of the astrolabe of the Prague astronomical clock. The result of this work will by a didactic instrument which will help users discover and understand the astronomical clock. The task is to create a realistic three-dimensional computer model of the astronomical clock and also to implement all movement of the clock. The application will offer three-dimensional realistic visualization of the astronomical clock, description of the clock's parts, and projection of the celestial sphere on the astronomical dial and information which can be read from the dial. The application will provide a possibility to see animation of the astronomical clock and also to set the clock to an arbitrary time during the year.
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Shell galaxies: kinematical signature of shells, satellite galaxy disruption and dynamical friction
Ebrová, Ivana ; Jungwiert, Bruno (advisor) ; Šubr, Ladislav (referee) ; Šolc, Martin (referee)
Title: Shell galaxies: kinematical signature of shells, satellite galaxy disruption and dynamical friction Author: Ivana Ebrová Department / Institute: Astronomical Institute of the Academy of Sciences of the Czech Republic Supervisor of the doctoral thesis: RNDr. Bruno Jungwiert, Ph.D., Astronomical Institute of the Academy of Sciences of the Czech Republic Abstract: Stellar shells observed in many giant elliptical and lenticular as well as a few spiral and dwarf galaxies presumably result from radial minor mergers of galaxies. We show that the line-of-sight velocity distribution of the shells has a quadruple-peaked shape. We found simple analytical expressions that connect the positions of the four peaks of the line profile with the mass distribution of the galaxy, namely, the circular velocity at the given shell radius and the propagation velocity of the shell. The analytical expressions were applied to a test-particle simulation of a radial minor merger, and the potential of the simulated host galaxy was successfully recovered. Shell kinematics can thus become an independent tool to determine the content and distribution of dark matter in shell galaxies up to ~100 kpc from the center of the host galaxy. Moreover we investigate the dynamical friction and gradual disruption of the cannibalized galaxy...
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Recent asteroid breakups and accretion of interplanetary dust on the Earth
Pokorný, Petr ; Vokrouhlický, David (advisor) ; Šolc, Martin (referee)
The major aim of the thesis is an analysis of an accretion of dust originating from breakup events of Emilkowalski and YC2 asterodial families. Using a numerical integrator we follow orbits of individual dust particles, some of which will result in an impact onto one of the planets in the Solar system. Employing some non-trivial transformation we compare recorded impacts onto the Earth to available dust measurements values acquired in antarctic ice-cores. We also analyse the dynamical e ffects of Poynting-Robertson e ffect and their influence on the dust particles of variable sizes.
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Protection of Personal Data
Šolc, Martin ; Millerová, Ivana (referee) ; Kopecký, Martin (referee)
This rigorous thesis deals with the protection of personal data. This is an issue relating to each of us, thereby personal data and its protection becomes very significant legal phenomenon. The thesis includes alongside the initial part, where a concept of personal data and a sense of its protection is described, also treatise on historical development of international law on protection of personal data and on constitutional ground too. The largest part is devoted to the Act on the Protection of Personal Data and its legal regulation of protection of personal data, which is also the main formal source of its legislation. It is followed by the part dedicated to the protection of personal data according to selected special laws. And the last part of the thesis is a treatise on the possibilities of judicial protection. The thesis strives for comprehensive and thoroughgoing analysis of protection of personal data in terms of generally binding legal regulations, and for the identification of weaknesses in the legislation on protection of personal data, as well as for its clear and logical submission eligible also for use of law laymen.
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