Kristopher Klein

Dr. Klein's research focuses on studying fundamental plasma phenomena that governs the dynamics of systems within our heliosphere as well as more distant astrophysical bodies. He has particular interest in identifying heating and energization mechanisms in turbulent plasmas, such as the Sun's extended atmosphere known as the solar wind, as well as evaluating the effects of the departure from local thermodynamic equilibrium on nearly collisionless plasmas which are ubiquitous in space environments. As part of this work, Prof. Klein is a co-developer of the Arbitrary Linear Plasma Solver (ALPS) numerical dispersion solver, an open source code used for quantifying the behavior of such non-equilibrium systems.

These systems are studied with a combination of analytic theory and numerical simulation, including large-scale nonlinear turbulence codes such as AstroGK, HVM, and gkeyll. These theoretical predictions are compared to in situ observations from spacecraft including NASA's Wind, MMS and Parker Solar Probe mission, as well as the upcoming HelioSwarm mission, which will fly nine spacecraft between the Earth and moon to characterize the transport and dissipation of turbulent energy in space plasmas. By comparing theory with local plasma measurements, we aim to answer a variety of questions about the behavior of plasma in our solar system.