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  • NAM2019
    • Registration
    • Key Dates & Outline Schedule
    • Practical Information
    • Exhibitors
    • Grants & Bursaries
    • Contacts
  • Science
    • Science Programme
    • Parallel Sessions
    • Plenary Talks
    • Community Session
    • Special Lunches
    • Posters
    • Presenter Guidelines
  • Social
    • What's On
    • Welcome Reception
    • RAS Awards Dinner
  • Media
  • Outreach
    • Outreach and Education Day
    • Fringe Event
    • School Visit Day
  • Lancaster
    • Travel
    • Accommodation
    • Childcare
    • Campus Map
    • About Lancaster
    • Code of Conduct

Programme by Session

Schedule

id
Tuesday
date time
PM1
Abstract
A 2D two-fluid MHD code to model partially-ionised plasma: calibration and a future benchmark

Abstract details

id
A 2D two-fluid MHD code to model partially-ionised plasma: calibration and a future benchmark
Date Submitted
2019-03-15 10:08:16
Linh
Le Phuong
Northumbria University
Current Developments in Numerical Astrophysics
Poster
L. Le Phuong (Northumbria University), S. Shelyag (Deakin University), G. J. J. Botha (Northumbria University), J. A. McLaughlin (Northumbria University)
In the lower solar atmosphere, there exists partially-ionised plasma and such an environment changes significantly the dynamics of the plasma-to-magnetic-field interaction. Appropriate numerical treatment of this requires a more complex description than single-fluid magnetohydrodynamics (MHD) can provide.

A 2D two-fluid MHD code is developed to simulate partially-ionised plasma. The code is validated through various standard tests to demonstrate a high level of accuracy and stability. These tests include the Sod-shock tube test in hydrodynamics, and the Brio-Wu shock and Orszag-Tang vortex test in MHD. To calibrate the two-fluid code, we benchmark against a 1D slow-mode MHD shock, known as the switch-off shock. Furthermore, we initiate the Orszag-Tang vortex test in the two-fluid setting, and present the results as a future benchmark test for 2D two-fluid tests.

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