F. Schmitz

发表

Theoretical chromospheres of late type stars. I. Acoustic energy generation.

A. Renzini, C. Cacciari, P. Ulmschneider, 1977 .

Solutions for the equilibrium of static isothermal gas clouds with poloidal magnetic fields

P. Baureis, F. Schmitz, R. Ebert, 1989 .

Equilibrium structures of differentially rotating self-gravitating gases

F. Schmitz, 1988 .

The effect of a poloidal magnetic field on the stability of a rotating self-gravitating disc

F. Schmitz, 1987 .

The stability of differentially rotating self-gravitating gas clouds. I - an approximation method and its application to isothermal configurations

F. Schmitz, 1986 .

An exact solution for a rotating selfgravitating gas mass with oscillatory density

F. Schmitz, R. Ebert, 1986 .

The structure, stability, and form of marginally stable axisymmetric perturbations of rotating gas clouds with simple conformal density distributions. I - General features and analytical solutions

F. Schmitz, 1984 .

The influence of the solar atmospheric stratification on the structure of the acoustic wave field

F. Deubner, S. Steffens, F. Schmitz, 1997 .

Radial stellar oscillations under the influence of the dynamics of the atmosphere — a one-dimensional approach I. Linear adiabatic oscillations of a special model

F. Schmitz, Theoretische Physik, 2000 .

On the propagation of linear 3-D hydrodynamic waves in plane non-isothermal atmospheres

B. Fleck, F. Schmitz, 1994 .

Towards an explanation of features in the diagnostic diagram of a model atmosphere I. Linear wave equations with convenient invariants

B. Fleck, F. Schmitz, 2003 .

The 3-min oscillations of the solar chromosphere―a basic physical effect?

B. Fleck, F. Schmitz, 1991 .

A closed solution for an adiabatic sound wave in a grey radiative equilibrium atmosphere

F. Schmitz, 1984 .