Erratum: ‘‘Effects of secondary and thermionic electron emission on the collector and source sheaths of a finite ion temperature plasma using kinetic theory and numerical simulation’’ [Phys. Fluids B 5, 631 (1993)]

1993 ◽  
Vol 5 (6) ◽  
pp. 1926-1926
Author(s):  
L. A. Schwager
Author(s):  
S Bair

A thorough characterization of all viscous flow properties relevant to steady simple shear was carried out for five liquid lubricants of current interest to tribology. Shear stresses were generated to values significant to concentrated contact lubrication. Two types of non-Newtonian response were observed: shear-thinning as a power-law fluid and near rate-independence. Functions and parameters were obtained for the temperature and pressure dependence of the viscosity and of the time constant for the Carreau-Yasuda equation. Results are consistent with free volume and kinetic theory, but directly contradict many assumptions currently utilized for numerical simulation and for extracting rheological properties from contact measurements.


1980 ◽  
Vol 175 (2-3) ◽  
pp. 293-296 ◽  
Author(s):  
F.E. Cecil ◽  
Lek Keah Len ◽  
R.J. Peterson

2020 ◽  
Vol 493 (4) ◽  
pp. 5761-5772 ◽  
Author(s):  
Takumi Ohmura ◽  
Mami Machida ◽  
Kenji Nakamura ◽  
Yuki Kudoh ◽  
Ryoji Matsumoto

ABSTRACT We present the results of two-temperature magnetohydrodynamic simulations of the propagation of sub-relativistic jets of active galactic nuclei. The dependence of the electron and ion temperature distributions on the fraction of electron heating, fe, at the shock front is studied for fe = 0, 0.05, and 0.2. Numerical results indicate that in sub-relativistic, rarefied jets, the jet plasma crossing the terminal shock forms a hot, two-temperature plasma in which the ion temperature is higher than the electron temperature. The two-temperature plasma expands and forms a backflow referred to as a cocoon, in which the ion temperature remains higher than the electron temperature for longer than 100 Myr. Electrons in the cocoon are continuously heated by ions through Coulomb collisions, and the electron temperature thus remains at Te > 109 K in the cocoon. X-ray emissions from the cocoon are weak because the electron number density is low. Meanwhile, X-rays are emitted from the shocked intracluster medium (ICM) surrounding the cocoon. Mixing of the jet plasma and the shocked ICM through the Kelvin–Helmholtz instability at the interface enhances X-ray emissions around the contact discontinuity between the cocoon and shocked ICM.


2014 ◽  
Vol 211 (10) ◽  
pp. 2238-2243 ◽  
Author(s):  
S. Elfimchev ◽  
Sh. Michaelson ◽  
R. Akhvlediani ◽  
M. Chandran ◽  
H. Kaslasi ◽  
...  

2012 ◽  
Vol 49 (8) ◽  
pp. 083201
Author(s):  
徐斌 Xu Bin ◽  
伍晓宇 Wu Xiaoyu ◽  
凌世全 Ling Shiquan ◽  
罗烽 Luo Feng ◽  
杜晨林 Du Chenlin ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document