Theoretical or Mathematical/ dusty plasmasKorteweg-de Vries equationplasma ion acoustic wavesplasma kinetic theoryplasma shock wavesplasma simulation/ dust ion acoustic shock wavescollisionless dusty plasmanonadiabatic dust charge variationdissipative effect...
Rarefaction Shock Waves in Collisionless Plasma with Electronic BeamRarefaction Shock Waves in Collisionless Plasma with Electronic Beamelectromagnetic perturbationquasinormal frequenciesWKB approximationWe show that an electron beam passing through a collisionless plasma of "cold" ions and "hot" Boltzmann electr...
Collisionless Shock Waves in interstellarTopics, Hot
This value is much higher than the electron temperature and results in a local plasma 尾 between 0.3 and 5. In this initial plasma stationary collisionless shock waves with Mach numbers between 1.5 and 5 are observed. The snow-plough model is used to derive conditions for the stationary state...
R. A. Chevalier, Magnetic field amplification in interstellar collisionless shock waves, Na- ture266 (1977) 701-+. doi:10.1038/266701a0.Chevalier, R. 1977a. Nature, 266 , 701.Chevalier RA (1977) Magnetic field amplification in interstellar collisionless shock waves. Nature 266:701-+...
Tidman DA, Krall NA (1971) Shock waves in collisionless plasmas. Wiley-Interscience, New York Google Scholar Treumann RA (2009) Fundamentals of collisionless shocks for astrophysical application, 1. Non-relativistic shocks. Astron Astrophys Rev 19:409–535. doi:10.1007/s00159-009-0024-2 ADS...
Charged particles can be accelerated to high energies by collisionless shock waves in astrophysical environments, such as supernova remnants. By interacting with the magnetized ambient medium, these shocks can transfer energy to particles. Despite increasing efforts in the characterization of these shocks...
plasma shock wavesrelativistic plasmasThe filamentation instability (sometimes also referred to as "Weibel") is a key process in many astrophysical scenario. In the Fireball model for gamma ray bursts, this instability is believed to mediate collisionless shock formation from the collision of two ...
Particle acceleration at planetary bow shock waves We can extend our understanding of collisionless shocks by comparing their behaviour in a variety of plasma conditions at several different planets. One pr... MM Hoppe,CT Russell - 《Nature》 被引量: 93发表: 1982年 Pressure wave generated by th...
Low Frequency Waves at and Upstream of Collisionless Shocks 2016, Low-Frequency Waves in Space Plasmas Shocklets, SLAMS, and field-aligned ion beams in the terrestrial foreshock 2013, Journal of Geophysical Research: Space Physics The foreshock 2005, Space Science Reviews Quasi-monochromatic ULF for...