Associate Professor Office: Cramer Hall 2040 Phone: 256-961-7321 Email: email@example.com Education B.S. 1982, University of Stellenbosch, South Africa M.S. 1987, Northwest University, South Africa Ph.D. 1990, Northwest University, South Africa Research interests Field: Heliospheric space plasma physics - energetic charged particle behavior. Basic interests Basic kinetic transport theory of energetic charged particles in tenuous nonuniform high-conductivity collisionless plasma flows, Quasi-linear, and nonlinear kinetic theory of energetic charged particle scattering and stochastic acceleration in turbulent low-frequency electromagnetic fields of tenuous collisionless high conductivity plasmas, Kinetic theory of energetic charged particle acceleration at collisionless shocks, Magnetohydromagnetic theory of large-scale plasma flow, Magnetohydromagnetic turbulence and weak turbulence kinetic theory. Specific interests All aspects of suprathermal (energetic) charged particle transport and acceleration in the solar wind plasma. Particle populations of interest include solar energetic particles, pickup ions, anomalous cosmic rays and galactic cosmic rays, Test particle and self-consistent finite difference and finite volume simulations of suprathermal charged particle transport and acceleration in the solar wind plasma, The acceleration of solar energetic particles at fast coronal mass ejection driven traveling bow shocks, including self-consistent wave generation, The acceleration of interstellar pickup ions at the heliospheric termination shock, including modification of the shock structure by the accelerated pickup ions (see figure), The acceleration of superthermal particles in a “sea” of contracting and merging (reconnecting) small-scale magnetic flux ropes in the supersonic solar wind plasma and in the corona, The non-diffusive parallel and perpendicular transport of energetic charged particles in intermittent low-frequency solar wind magnetic field turbulence including propagation of anomalous and galactic cosmic rays through the heliopause. Comparison of Voyager 2 energetic ion spectral data behind the heliospheric termination shock as adapted from Decker et al., 2008 (left panel) with a kinetic focused transport theory simulation (right panel) of the shock accelerated interstellar pickup proton spectrum (left panel). The simulation illustrates the importance of including perpendicular diffusion of accelerated pickup ions across the termination shock due to magnetic field-line random walk in the shock acceleration process. The work was published in Astrophysical Journal Letters in 2013 with current Ph.D. student Aaron Arthur as the lead author. Current graduate students Aaron Arthur Ph.D. expected 2015 Dissertation: "A focused transport model for solar energetic particle acceleration at fast traveling shocks driven by extreme coronal mass ejections". Junye Ye Ph.D. expected 2015 Dissertation: "A kinetic transport model for interstellar pickup ion acceleration at the heliospheric termination shock". Past graduate students Edmont Smith M.S. 2010 (non-thesis) Selected recent publications le Roux, J. A., Zank, G. P., Webb, G.M., Khabarova, O. (2015). A Kinetic Transport Theory for Particle Acceleration and Transport in Regions of Multiple Contracting and Reconnecting Inertial-scale Flux Ropes. The Astrophysical Journal, 801, 112. 24 pages. Xu, F., Li, G., Zhao, L., Zhang, Y., Khabarova, O., Miao, B., Le Roux, J. A. (2015). Angular Distribution of Solar Wind Magnetic Field Vector at 1 AU. The Astrophysical Journal, 801, 58. Diffusive Shock Acceleration and Reconnection Acceleration Processes by G P Zank, P Hunana, P Mostafavi, J A le Roux, G Li, G M Webb, O Khabarova, A C Cummings, E C Stone, & R B Decker, Astrophysics J, 814, 137, 23 pp, 2015. Small-scale Magnetic Islands in the Solar Wind and Their Role in Particle Acceleration. I. Dynamics of Magnetic Islands Near the Heliospheric Current Sheet by O Khabarova, G P Zank, G Li, J A le Roux, G M Webb, A Dosch, O E Malandraki,, Astrophys. J., 808, 181, 13 pp, 2015. Energetic Particle Anisotropies at the Heliospheric Boundary. II. Transient Features and Rigidity Dependence by V Florinski, E C Stone, A C Cummings, J A le Roux, J. A Astrophysics J., 803, 47, 8 pp, 2015. Acceleration by Small-scale Solar Wind Flux Ropes by J A le Roux, G Webb, G P Zank, O Khabarova, Energetic Ion, J. Physics: Conf. Series, 642, 012015, 2015. Particle acceleration by combined diffusive shock acceleration and downstream multiple magnetic island acceleration, by G P Zank, P Hunana, P Mostafavi, J A le Roux, G Li, G M Webb, O Khabarova, J. Physics: Conf. Series, 642, 012031, 2015. Cosmic ray transport near the heliopause by R D Strauss, H Fichtner, M S Potgieter, J A le Roux, X Luo, J. Physics: Conf. Series, 642, 012026, 2015. Alouani-Bibi, F., and le Roux, J. A., Transport of cosmic-ray protons in intermittent heliopsheric turbulence: Model and simulations, Astrophysical Journal, 781, 93 (2014). Zank, G. P., Le Roux, J. A., Webb, G.M., Dosch, A., Khabarova, O. (2014). Particle Acceleration via Reconnection Processes in the Supersonic Solar Wind. The Astrophysical Journal, 797, 28. Recent grants and contracts The implication of non-Gaussian magnetic field-line wandering for the anomalous diffusion and shock acceleration of cosmic rays (NASA HSR) - $407,423. Anomalous diffusion in the collisionless solar wind plasma (NSF-DOE) - $438,228. Modeling the radial dependence of the shock acceleration of solar energetic particles from the corona to Earth with a time-dependent focused transport model (NASA LWS) - $439,902. Probing the physics of the heliopause region (NASA NNH13ZDA001N-HSR) - $396,020.