Covers the modeling of fluid instabilities with linear perturbation theory and explores the origin of unpredictability in turbulence through the Navier-Stokes equations.
Explores radiative heat transfer equilibrium between walls and isotropic scattering medium, optical thickness, Monte Carlo method, and analytical solutions.
Explores the characteristics of typical plasmas from interstellar space to solar corona, discussing temperature, number density, collision processes, and properties.
