@unpublished{MeisterDziourkevich2000,
  author    = {Meister, Claudia-Veronika and Dziourkevich, Natalia S.},
  title     = {Temperature-anisotropy driven mirror waves in space plasma},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-14977},
  year      = {2000},
  abstract  = {In this paper an analysis of the excitation conditions of mirror waves is done, which propagate parallel to an external magnetic field. There are found analytical expressions for the dispersion relations of the waves in case of different plasma conditions. These relations may be used in future to develop the nonlinear theory of mirror waves. In comparison with former analytical works, in the study the inuence of the magnetic field and nite temperatures of the ions parallel to the magnetic field are taken into account. Application is done for the earth's magnetosheath.},
  language  = {en}
}
@unpublished{VolosevichMeister2000,
  author    = {Volosevich, Alexandra and Meister, Claudia-Veronika},
  title     = {Nonlinear electrostatic ion-acoustic waves in the solar atmosphere},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-14968},
  year      = {2000},
  abstract  = {Basing on recent solar models, the excitation of ion-acoustic turbulence in the weaklycollisional, fully and partially-ionized regions of the solar atmosphere is investigated. Within the frame of hydrodynamics, conditions are found under which the heating of the plasma by ion-acoustic type waves is more effective than the Joule heating. Taking into account wave and Joule heating effects, a nonlinear differential equation is derived, which describes the evolution of nonlinear ion-acoustic waves in the collisional plasma.},
  language  = {en}
}
@unpublished{ZakharovMeister2000,
  author    = {Zakharov, Venjamin E. and Meister, Claudia-Veronika},
  title     = {Acceleration and heating in the auroral magnetosphere by current driven electrostatic ion cyclotron turbulence},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-14959},
  year      = {2000},
  abstract  = {A numerical MHD model is developed to investigate acceleration and heating of both thermal and auroral plasma. This is done for magnetospheric flux tubes in which intensive field aligned currents flow. To give each of these tubes, the empirical Tsyganenko model of the magnetospheric field is used. The parameters of the background plasma outside the flux tube as well as the strength of the electric field of magnetospheric convection are given. Performing the numerical calculations, the distributions of the plasma densities, velocities, temperatures, parallel electric field and current, and of the coefficients of thermal conductivity are obtained in a self-consistent way. It is found that EIC turbulence develops effectively in the thermal plasma. The parallel electric field develops under the action of the anomalous resistivity. This electric field accelerates both the thermal and the auroral plasma. The thermal turbulent plasma is also subjected to an intensive heating. The increase of the plasma of the Earth's ionosphere. Besides, studying the growth and dispersion properties of oblique ion cyclotron waves excited in a drifting magnetized plasma, it is shown that under non-stationary conditions such waves may reveal the properties of bursts of polarized transverse electromagnetic waves at frequencies near the patron gyrofrequency.},
  language  = {en}
}