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An improved ten-moment closure for reconnection and instabilities

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/5.0012067· OSTI ID:1843022
 [1];  [2];  [2];  [3]
  1. Princeton Univ., NJ (United States); Univ. of Maryland, College Park, MD (United States); University of Maryland, College Park
  2. Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)
  3. Princeton Univ., NJ (United States); Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)

The integration of kinetic effects in fluid models is important for global simulations of Earth's magnetosphere. The use of the two-fluid ten-moment model, which includes the pressure tensor for both species, has had some success in simulating Ganymede and Mercury with a simple closure model. Here, we discuss a heat flux closure which accounts for some limitations of the earlier work while remaining computationally tractable. Comparisons with kinetic simulations for magnetic reconnection and lower-hybrid drift instabilities show good agreement with kinetic results and improvements on previous closure models.

Research Organization:
Univ. of Maryland, College Park, MD (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
SC0016278
OSTI ID:
1843022
Alternate ID(s):
OSTI ID: 1648584
Journal Information:
Physics of Plasmas, Journal Name: Physics of Plasmas Journal Issue: 8 Vol. 27; ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English

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