PTYS/LPL Faculty
Kristopher Klein
Assistant Professor
Solar and Heliospheric Research, Theoretical Astrophysics Research, Parker Solar Probe
Ph.D., 2013, University of Iowa
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Kuiper 431
Years with LPL: 2017
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.
These systems are studied with a combination of analytic theory and numerical simulation, including large-scale nonlinear turbulence codes such as AstroGK and HVM. These theoretical predictions are compared to in situ observations from spacecraft including NASA's Wind and MMS and the upcoming Parker Solar Probe mission. By comparing theory with local plasma measurements, we aim to answer a variety of questions about the behavior of plasma in our solar system.
View LPL Evening Lecture from September 12, 2018, Visiting Our Sun: Unraveling the Mysteries of the Solar Atmosphere using Parker Solar Probe
Current Grants
•Solar Wind Electrons Alphas and Protons (SWEAP): NASA's Parker Solar Probe mission; member of Science, Theory, and Modeling Team
•Assessing the Relative Importance of Stochastic and Resonant Ion Heating the Solar Wind, NASA Heliophysics Supporting Research Program
•Non-Maxwellian Distribution Functions in the Solar Wind: Dispersion Relations and Instabilities, NASA Heliophysics Supporting Research Program
Current PTYS Graduate Students
Current Postdocs
Complete publications list available from: NASA ADS Author search: Kristopher G. Klein
Refereed publications (NASA ADS): Calendar Years 2017 and 2018
Hoppock, I. W., Chandran, B. D. G., Klein, K. G., Mallet, A., Verscharen, D. Stochastic proton heating by kinetic-Alfvén-wave turbulence in moderately high- plasmas 2018JPlPh..84f9015H
Vech, D., Klein, K. G., Kasper, J. C. Large-scale Control of Kinetic Dissipation in the Solar Wind 2018ApJ...863L...4V
Wilson, L. B., III, Stevens, M. L., Kasper, J. C., Klein, K. G., Maruca, B. A., Bale, S. D., Bowen, T. A., Pulupa, M. P., Salem, C. S. The Statistical Properties of Solar Wind Temperature Parameters Near 1 au 2018ApJS..236...41W
Vech, D., Mallet, A., Klein, K. G., Kasper, J. C. Magnetic Reconnection May Control the Ion-scale Spectral Break of Solar Wind Turbulence 2018ApJ...855L..27V
Howes, G. G., McCubbin, A. J., Klein, K. G. Spatially localized particle energization by Landau damping in current sheets produced by strong Alfvén wave collisions 2018JPlPh..84a9005H
Vech, D., Klein, K. G., Kasper, J. C. Nature of Stochastic Ion Heating in the Solar Wind: Testing the Dependence on Plasma Beta and Turbulence Amplitude 2017ApJ...850L..11V
Klein, K. G., Kasper, J. C., Korreck, K. E., Stevens, M. L. Applying Nyquist's method for stability determination to solar wind observations 2017JGRA..122.9815K
Howes, G. G., McCubbin, A. J., Klein, K. G. Using Field-Particle Correlations to Show that Landau Damping Leads to Spatially Intermittent Particle Energization in Current Sheets 2017APS..DPPNP11158
Klein, K. G., Howes, G. G., Tenbarge, J. M. Diagnosing collisionless energy transfer using field-particle correlations: gyrokinetic turbulence 2017JPlPh..83d5301K
Klein, K. G. Characterizing fluid and kinetic instabilities using field-particle correlations on single-point time series 2017PhPl...24e5901K
Howes, G. G., Klein, K. G., Li, T. C. Diagnosing collisionless energy transfer using field-particle correlations: Vlasov-Poisson plasmas 2017JPlPh..83a7002H
| Available files | Size | Created |
|---|---|---|
 Klein_Kristopher_CV.pdf | 55.89 KB | December 15, 2018 |
| Semester | Course | Day/Time | Location | Resources |
|---|---|---|---|---|
| Spring 2020 | PTYS 170A1-001 | |||
| Fall 2020 | PTYS 537-001 | |||
| Fall 2019 | PTYS 170A1-001 | TTH 12:30-1:45p.m. | Kuiper 308 |