
Jacob Bortnik is a recognized leader in nonlinear plasma wave interactions with charged particles in Earth’s radiation belts (the Van Allen belts). Relativistic electrons and energetic protons there can damage satellites, disrupting telecommunications and other services we have come to depend upon, and can endanger astronauts. Radiation belt fluxes are highly variable due to changes in the solar wind, which powers them. Understanding the physics of this variability to build accurate predictive models of “space weather” is a major goal of space science. The emergence of space-based internet, space tourism and the U.S. Space Force reveals that the need for such models is on the rise. A key factor responsible for the dynamic nature of the radiation belt fluxes is the interaction of energetic particles with plasma waves. Professor Bortnik has made some of the most significant advances in our understanding of such interactions, using theory, modeling, observations, laboratory and computer simulations, and machine learning.
Jacob theorized and then proved using data from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission that plasmaspheric hiss waves, a dominant contributor to outer-belt energetic particle losses and the reason for the two-belt structure of the radiation belts, are produced by the leakage of magnetospheric whistler waves produced by particle injections at larger radial distances. This solved a 40-year-old mystery on the origin of plasmaspheric hiss. His contributions to the understanding of how chorus waves drive the pulsating aurora, how lightning-generated whistlers can diffract and stay in the magnetosphere, and how electromagnetic ion cyclotron waves and magnetosonic waves can resonate nonlinearly with electrons to energize and scatter them have been seminal. He pioneered laboratory experiments at the University of California, Los Angeles, Large Plasma Device coupled with numerical simulations to show how nonlinear wave structures arise from wave-particle interactions under certain plasma conditions. He developed novel machine learning tools for reconstructing the spatial and temporal evolution of plasmas in the magnetosphere, which is only sparsely sampled by spacecraft. He has mentored dozens of students and early-career space physicists. He is generous with his time to both students and colleagues, making him a highly sought after adviser and collaborator. He has led the field as National Science Foundation’s Geospace Environment Modeling program chair, an associate editor of AGU journals and co-chair of international groups under the auspices of the International Union of Radio Science and the International Science Council’s Scientific Committee on Solar-Terrestrial Physics. His collaborative spirit and transformational research on wave-particle interactions have made an indelible mark in space science.
— Vassilis Angelopoulos
University of California, Los Angeles
Los Angeles, California