Unraveling the physics of the entire turbulent cascade of energy in space and astrophysical plasmas from the injection of energy at large scales to the dissipation of that energy into plasma heat at small scales, represents an overarching, open question in heliophysics and astrophysics. The fast cadence and high phase-space resolution of particle velocity distribution measurements on modern spacecraft missions, such as the recently launched Parker Solar Probe, presents exciting new opportunities for identifying turbulent dissipation mechanisms using in situ measurements of the particle velocity distributions and electromagnetic fields. Here we demonstrate how to use data from kinetic numerical simulations of plasma turbulence to create synt...
International audienceContext. The recently released spacecraft potential measured by the RPW instru...
International audienceThe description of the turbulent spectrum of magnetic fluctuations in the sola...
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Nuclear Science and Engineering...
How turbulent energy is dissipated in weakly collisional space and astrophysical plasmas is a major ...
The field-particle correlation technique utilizes single-point measurements to uncover signatures of...
The ability to understand the fundamental nature of the physics that governs the heliosphere require...
A leap forward in our understanding of particle energization in plasmas throughout the heliosphere i...
The availability of large in-situ datasets makes the solar wind an excellent astrophysical laborator...
Turbulence is commonly observed in nearly collisionless heliospheric plasmas, including the solar wi...
The solar wind is a highly turbulent medium in which most of the energy is carried by Alfvénic fluct...
International audienceMagnetic turbulence in the solar wind has been studied since the beginning of ...
Wave-particle interactions in collisionless plasmas are fundamental processes by which energy is tra...
Spacecraft observations from the interplanetary medium of our solar system reveal the presence of a ...
International audienceContext. The recently released spacecraft potential measured by the RPW instru...
International audienceThe description of the turbulent spectrum of magnetic fluctuations in the sola...
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Nuclear Science and Engineering...
How turbulent energy is dissipated in weakly collisional space and astrophysical plasmas is a major ...
The field-particle correlation technique utilizes single-point measurements to uncover signatures of...
The ability to understand the fundamental nature of the physics that governs the heliosphere require...
A leap forward in our understanding of particle energization in plasmas throughout the heliosphere i...
The availability of large in-situ datasets makes the solar wind an excellent astrophysical laborator...
Turbulence is commonly observed in nearly collisionless heliospheric plasmas, including the solar wi...
The solar wind is a highly turbulent medium in which most of the energy is carried by Alfvénic fluct...
International audienceMagnetic turbulence in the solar wind has been studied since the beginning of ...
Wave-particle interactions in collisionless plasmas are fundamental processes by which energy is tra...
Spacecraft observations from the interplanetary medium of our solar system reveal the presence of a ...
International audienceContext. The recently released spacecraft potential measured by the RPW instru...
International audienceThe description of the turbulent spectrum of magnetic fluctuations in the sola...
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Nuclear Science and Engineering...