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Title: The ecology of flows and drift wave turbulence in CSDX: A model

Abstract

This paper describes the ecology of drift wave turbulence and mean flows in the coupled drift-ion acoustic wave plasma of a CSDX linear device. A 1D reduced model that studies the spatiotemporal evolution of plasma mean density $$\bar{n}$$, and mean flows $$\bar{v}$$y and $$\bar{v}$$z, in addition to fluctuation intensity ε, is presented. Here, ε = n ~ 2 + ( Φ ~ ) 2 + v ~ z 2 is the conserved energy field. The model uses a mixing length lmix inversely proportional to both axial and azimuthal flow shear. This form of lmix closes the loop on total energy. The model self-consistently describes variations in plasma profiles, including mean flows and turbulent stresses. It investigates the energy exchange between the fluctuation intensity and mean profiles via particle flux n ~ v ~ x and Reynolds stresses v ~ x v ~ y and v ~ x v ~ z Acoustic coupling breaks parallel symmetry and generates a parallel residual stress Π res xz . The model uses a set of equations to explain the acceleration of $$\bar{v}_y$$ and $$\bar{v}_z$$ via Π x y r e s n - and Π x y r e s n - . Flow dynamics in the parallel direction are related to those in the perpendicular direction through an empirical coupling constant σVT. This constant measures the degree of symmetry breaking in the 〈$$k_mk_z$$〉 correlator and determines the efficiency of ∇$$\bar{n}$$ in driving $$\bar{v}_z$$. The model also establishes a relation between ∇$$\bar{v}_y$$ and ∇$$\bar{v}_z$$, via the ratio of the stresses Π res xy and Π res xz . When parallel to perpendicular flow coupling is weak, axial Reynolds power P x z R e = - v ~ x v ~ z v - z is less than the azimuthal Reynolds power P x y R e = - v ~ x v ~ y v - y ∇$$\bar{v}_y$$. The model is then reduced to a 2-field predator/prey model where $$\bar{v}_z$$ is parasitic to the system and fluctuations evolve self-consistently. Finally, turbulent diffusion in CSDX follows the scaling: D CSDX = D B ρ * 0.6 , where DB is the Bohm diffusion coefficient and ρ* is the ion gyroradius normalized to the density gradient | n - / n - | - 1

Authors:
 [1];  [2];  [3]
  1. Univ. of California, San Diego, CA (United States). Center for Energy Research
  2. Univ. of California, San Diego, CA (United States). Center for Energy Research, Center for Astrophysics and Space Sciences; Center for Fusion Sciences, Southwestern Inst. of Physics, Chengdu, Sichuan (China)
  3. Univ. of California, San Diego, CA (United States). Center for Energy Research; Center for Fusion Sciences, Southwestern Inst. of Physics, Chengdu, Sichuan (China)
Publication Date:
Research Org.:
Univ. of California, San Diego, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
OSTI Identifier:
1524572
Alternate Identifier(s):
OSTI ID: 1420214
Grant/Contract Number:  
FG02-04ER54738
Resource Type:
Accepted Manuscript
Journal Name:
Physics of Plasmas
Additional Journal Information:
Journal Volume: 25; Journal Issue: 2; Journal ID: ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY

Citation Formats

Hajjar, R. J., Diamond, P. H., and Tynan, G. R. The ecology of flows and drift wave turbulence in CSDX: A model. United States: N. p., 2018. Web. doi:10.1063/1.5018320.
Hajjar, R. J., Diamond, P. H., & Tynan, G. R. The ecology of flows and drift wave turbulence in CSDX: A model. United States. https://doi.org/10.1063/1.5018320
Hajjar, R. J., Diamond, P. H., and Tynan, G. R. Thu . "The ecology of flows and drift wave turbulence in CSDX: A model". United States. https://doi.org/10.1063/1.5018320. https://www.osti.gov/servlets/purl/1524572.
@article{osti_1524572,
title = {The ecology of flows and drift wave turbulence in CSDX: A model},
author = {Hajjar, R. J. and Diamond, P. H. and Tynan, G. R.},
abstractNote = {This paper describes the ecology of drift wave turbulence and mean flows in the coupled drift-ion acoustic wave plasma of a CSDX linear device. A 1D reduced model that studies the spatiotemporal evolution of plasma mean density $\bar{n}$, and mean flows $\bar{v}$y and $\bar{v}$z, in addition to fluctuation intensity ε, is presented. Here, ε=〈n~2+(∇⊥Φ~)2+v~z2〉 is the conserved energy field. The model uses a mixing length lmix inversely proportional to both axial and azimuthal flow shear. This form of lmix closes the loop on total energy. The model self-consistently describes variations in plasma profiles, including mean flows and turbulent stresses. It investigates the energy exchange between the fluctuation intensity and mean profiles via particle flux 〈n~v~x〉 and Reynolds stresses 〈v~xv~y〉 and 〈 v~xv~z〉 Acoustic coupling breaks parallel symmetry and generates a parallel residual stress Π res xz . The model uses a set of equations to explain the acceleration of $\bar{v}_y$ and $\bar{v}_z$ via Πxyres∝∇n- and Πxyres∝∇n-. Flow dynamics in the parallel direction are related to those in the perpendicular direction through an empirical coupling constant σVT. This constant measures the degree of symmetry breaking in the 〈$k_mk_z$〉 correlator and determines the efficiency of ∇$\bar{n}$ in driving $\bar{v}_z$. The model also establishes a relation between ∇$\bar{v}_y$ and ∇$\bar{v}_z$, via the ratio of the stresses Π res xy and Π res xz . When parallel to perpendicular flow coupling is weak, axial Reynolds power PxzRe=-〈v~xv~z〉∇v-z is less than the azimuthal Reynolds power PxyRe=-〈v~xv~y〉∇v-y∇$\bar{v}_y$. The model is then reduced to a 2-field predator/prey model where $\bar{v}_z$ is parasitic to the system and fluctuations evolve self-consistently. Finally, turbulent diffusion in CSDX follows the scaling: DCSDX=DBρ*0.6, where DB is the Bohm diffusion coefficient and ρ* is the ion gyroradius normalized to the density gradient |∇n-/n-|-1},
doi = {10.1063/1.5018320},
journal = {Physics of Plasmas},
number = 2,
volume = 25,
place = {United States},
year = {Thu Feb 01 00:00:00 EST 2018},
month = {Thu Feb 01 00:00:00 EST 2018}
}

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Free Publicly Available Full Text
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Cited by: 5 works
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Figures / Tables:

FIG. 1 FIG. 1: A schematic of the ecology of drift wave turbulence, zonal, and axial flows. The first feedback loop relates the drift waves to the zonal flows via (~vx~vy). A second feedback loop exists as a result of a potential relation between $\bar{v}$y and $\bar{v}$z. The second loop relates themore » fluctuations to both mean flows.« less

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