Collective processes and shock waves in a rarefied plasma
Approximation methods applied to collective processes, plasma-particle interaction, and shock waves in rarefied plasma
SEARCH · Search NASA
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Approximation methods applied to collective processes, plasma-particle interaction, and shock waves in rarefied plasma
Stability limits for longitudinal waves in ion beam-plasma interaction
Solar wind properties from space probe data noting interaction with Earth magnetosphere
Hydromagnetic whistlers considered as overlapping wavetrains generated by particle interaction and propagating along field aligned paths in magnetosphere
We propose novel numerical schemes based on the Boris method in curved spacetime, incorporating both hadronic and radiative interactions for the first time. Once the proton has lost significant energy due to radiative and hadronic losses, and its gyroradius has decreased below typical scales on which the electromagnetic field varies, we apply a guiding center approximation (GCA). We fundamentally simulate collision processes either with a Monte-Carlo method or, where applicable, as a continuous energy loss, contingent on the local optical depth. To test our algorithm for the first time combining the effects of electromagnetic, gravitational, and radiation fields including hadronic interactions, we simulate highly relativistic protons traveling through various electromagnetic fields and proton backgrounds. We provide unit tests in various spatially dependent electromagnetic and gravitational fields and background photon and proton distributions, comparing the trajectory against analytic results. We propose that our method can be used to analyze hadronic interactions in black hole accretion disks, jets, and coronae to study the neutrino abundance from active galactic nuclei.
Recent experimental demonstrations of ignition and target gain in inertial confinement fusion (ICF) have stimulated interest in exploring the fundamental physics of violent deuterium-tritium (DT) burn in high-gain ICF targets. A significant DT-burn fraction is a necessary condition for high energy gain and large neutron yields (>100MJ). Using classical molecular-dynamics (MD) simulations and a hybrid fluid-kinetic model, we examine how a large fraction of low-energy 𝛼 particles can kick D and T ions out of equilibrium in high-gain ICF targets. The MD results suggest that (1) temperatures of 𝑇 𝐷 and 𝑇 𝑇 can differ by as much as ∼20% of their mean temperature and (2) the deviation of the DT energy distribution from the Maxwell-Boltzmann function can exceed ∼30%. Some of these MD observations, such as the preferential heating of D ions by low-energy 𝛼 particles and the temperature separation, can be explained by a proposed hybrid fluid-kinetic model. Furthermore, the implication of such nonequilibrium effects on the DT reactivity is also discussed.
Microstructure of disordered hydromagnetic medium in collisionless limit
Pair collisions of metastable helium atoms in plasma
Charged particles interaction with turbulent plasma
Excitation and ionization collision parameters in plasmas involving electrons, atoms and ions at thermal energies
Equations for plasma waves produced by arbitrary current source in partly ionized gas with no steady magnetic field
Random plasma magnetic fields caused by electrons coming closer to plasma atom than mean interelectron distance and by electrons that pass at or beyond this distance
Arc model describing symptomatic behavior of fluctuating mode when axial gas flow is superimposed on electric arc
Laboratory scale model simulation of effect of solar wind on magnetosphere by propelling plasma stream into dipole magnetic field - time history of magnetospheric cavity
Collision interaction of energetic test electrons with plasma - expressions for energy loss rate and distribution of losses
Interaction of energetic test electrons with dense high temperature plasma and energy dissipation distribution
Mariner II investigations of relationship between high energy particles in space and solar plasma
Scattering of test particle by enhanced electric field fluctuations in plamsa containing nonthermal electrons