Publications by authors named "Craig Pollock"

We report results in the development and testing of a low resource tophat electrostatic analyzer (ESA) for space plasma measurements. This device has been additively manufactured (3D-printed) using fused deposition modeling. The classic tophat design is composed of four plastic pieces, without any surface coatings.

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Wave-particle resonance, a ubiquitous process in the plasma universe, occurs when resonant particles observe a constant wave phase to enable sustained energy transfer. Here, we present spacecraft observations of simultaneous Landau and anomalous resonances between oblique whistler waves and the same group of protons, which are evidenced, respectively, by phase-space rings in parallel-velocity spectra and phase-bunched distributions in gyrophase spectra. Our results indicate the coupling between Landau and anomalous resonances via the overlapping of the resonance islands.

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Turbulent energy dissipation is a fundamental process in plasma physics that has not been settled. It is generally believed that the turbulent energy is dissipated at electron scales leading to electron energization in magnetized plasmas. Here, we propose a micro accelerator which could transform electrons from isotropic distribution to trapped, and then to stream (Strahl) distribution.

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Shocks are one of nature's most powerful particle accelerators and have been connected to relativistic electron acceleration and cosmic rays. Upstream shock observations include wave generation, wave-particle interactions and magnetic compressive structures, while at the shock and downstream, particle acceleration, magnetic reconnection and plasma jets can be observed. Here, using Magnetospheric Multiscale (MMS) we show in-situ evidence of high-speed downstream flows (jets) generated at the Earth's bow shock as a direct consequence of shock reformation.

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Article Synopsis
  • NASA's Magnetospheric Multi-Scale (MMS) mission investigates the behavior of plasma turbulence, focusing on how particles are accelerated and heated within this environment.
  • The study develops a new kinetic theory to understand magnetic cavities, crucial structures for energy dynamics in plasma.
  • By using data from multiple MMS spacecraft, researchers can validate their theory through predictive modeling, demonstrating that these magnetic cavities are self-organized structures similar to those observed in laboratory settings.
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A familiar problem in space and astrophysical plasmas is to understand how dissipation and heating occurs. These effects are often attributed to the cascade of broadband turbulence which transports energy from large scale reservoirs to small scale kinetic degrees of freedom. When collisions are infrequent, local thermodynamic equilibrium is not established.

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Article Synopsis
  • The study estimates the turbulent energy-cascade rate using a third-order law from Hall-magnetohydrodynamics (MHD) and analyzes both Hall and MHD contributions to energy flux.
  • By comparing Magnetospheric Multiscale (MMS) data from the magnetosheath and solar wind with simulation results, researchers confirm that MMS observations show a clear inertial range at large MHD scales, primarily influenced by the MHD flux.
  • The findings reveal that even at smaller scales, the MHD contribution to energy transfer is more significant than previously believed, with the Hall term's role becoming more pronounced in high plasma beta conditions.
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Turbulence is a fundamental physical process through which energy injected into a system at large scales cascades to smaller scales. In collisionless plasmas, turbulence provides a critical mechanism for dissipating electromagnetic energy. Here we present observations of plasma fluctuations in low- turbulence using data from NASA's Magnetospheric Multiscale mission in Earth's magnetosheath.

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Microchannel plate (MCP) detectors provide a mechanism to produce a measureable current pulse (∼0.1 mA over several nanoseconds) when stimulated by a single incident particle or photon. Reductions of the device's amplification factor (i.

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Alfvén waves are fundamental plasma wave modes that permeate the universe. At small kinetic scales, they provide a critical mechanism for the transfer of energy between electromagnetic fields and charged particles. These waves are important not only in planetary magnetospheres, heliospheres and astrophysical systems but also in laboratory plasma experiments and fusion reactors.

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Article Synopsis
  • The study compares geometric factors (GF) from computer simulations and lab measurements for NASA's new Dual Electron Spectrometer (DES) used in the Magnetospheric Multiscale mission.
  • Particle simulations are crucial in designing and calibrating electrostatic analyzers, as they help to identify and reduce systematic errors common in lab settings.
  • The researchers derived new equations for calculating GF and demonstrated their applicability to the DES instrument, showing consistent results between simulations and laboratory measurements.
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