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  1. Orbit Dynamics, Stability and Chaos in Planetary Systems

    Let us start with a problem of dynamical biology, which was posed about 800 years ago by Fibonacci1
    Rudolf Dvorak, Florian Freistetter in Chaos and Stability in Planetary Systems
    Chapter
  2. 4 Continuous-time Systems: Tracking Control

    In this chapter we treat the problem of H∞ tracking with stochastic multiplicative white noise. We extend the work of [98], which does not involve...
    Chapter
  3. Basics of Plasma Physics

    Basic properties of plasmas are introduced, which are valid for an extremely wide range of plasma parameters. Plasmas are classified by different...
    U. Schumacher in Plasma Physics
    Chapter
  4. Strongly Coupled Plasmas

    We give a brief introduction into the basic many-particle effectes in strongly coupled plasmas and their theoretical treatment. Exemplary results are...
    R. Redmer in Plasma Physics
    Chapter
  5. Aerothermodynamics, Nonlinear Acoustics and the Meteorological Equations

    The study of low-Mach-number flows occurs in the general context of asymptotic modelling of fluid flows, and in a recent book (Zeytounian 2004, Chap....
    Radyadour Kh. Zeytounian in Topics in Hyposonic Flow Theory
    Chapter
  6. Planet Formation

    Motivating the study of planet formation is not difficult for any curious audience. One of the fundamental human questions is that of origins: “where...
    Chapter
  7. Magnetic Confinement

    This chapter describes the basic principles of magnetic confinement. The main representatives of magnetic confinement are the mirror machine, the...
    F. Wagner, H. Wobig in Plasma Physics
    Chapter
  8. 6 Shared Control

    Based on the successful implementations of the lateral balancing and tiltup motion, in this chapter, we are going to develop a shared control...
    Yangsheng Xu, Yongsheng Ou in Control of Single Wheel Robots
    Chapter
  9. 4 Compositional Modelling of Distributed-Parameter Systems

    The Hamiltonian formulation of distributed-parameter systems has been a challenging reserach area for quite some time. (A nice introduction,...
    Bernhard Maschke, Arjan van der Schaft in Advanced Topics in Control Systems Theory
    Chapter
  10. 6 Stochastic Passivity

    Passivity of deterministic linear systems plays an important role in network theory and in adaptive control. The fact that a system is passive...
    Chapter
  11. C Appendix: The Discrete DLMI Method

    We consider the following system: $$ x_{k+1}=A_kx_k + B_k w_k, \quad k=0,1,...
    Chapter
  12. Observation of Plasma Fluctuations

    The diagnostics of fluctuating plasma quantities and their evaluation is an important issue in the context of plasma waves, instabilities, and...
    O. Grulke, T. Klinger in Plasma Physics
    Chapter
  13. Low Temperature Plasmas

    Characteristic properties and generation mechanisms of low temperature plasmas in different gas discharges are presented. A special part is focussed...
    J. Meichsner in Plasma Physics
    Chapter
  14. Some Aspects of Low-Mach-Number External Flows

    In this chapter, we consider first, in Sect. 4.1, a detailed derivation of the Navier–Fourier initial–boundary–value problem for the Navier velocity...
    Radyadour Kh. Zeytounian in Topics in Hyposonic Flow Theory
    Chapter
  15. Clusters of Galaxies at High Redshift

    For a long time, the small number of clusters at z > 0.3 in the Abell survey catalogue and simulations of the standard CDM formation of large scale...
    Conference paper
  16. Velocity Dispersion Analysis of CNOC Clusters

    I present results of the analysis of the internal velocity dispersions,...
    Conference paper
  17. The Metal Enrichment History of Clusters of Galaxies

    The ratio of the total iron mass in the ICM to the total optical luminosity of the cluster (the iron mass-to-light-ratio) is the same for all...
    Conference paper
  18. Supernovae at High Redshift

    Distant supernovae provide a convenient tool for cosmology. As bright beacons with small variation in their peak luminosity Type Ia Supernovae can be...
    Conference paper
  19. The Galactic Bulge: Prospects for the VLT

    The central bulge of the Galaxy is 100 times closer than the nearest extragalactic bulge, that of M31. Until the era of 100m telescopes arrives, the...
    Conference paper
  20. The Old Population of the Magellanic Clouds

    The brightest old stars in the LMC are as faint as V=16 (V=16.5 in the SMC). The VLT with UVES or GIRAFFE will provide, for the first time, high...
    Conference paper
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