Fluid model
ShearAlfven
Shear-Alfvén part of LinearMHD with zero-flow equilibrium.
Overview
from linear MHD. It is useful when one wants to isolate Alfvénic propagation from the full linear MHD model.
Use cases
- isolated shear-Alfvén wave propagation
- verification of the ShearAlfven propagator
- reduced linear-MHD studies without compressibility
Governing equations
PDEs solved by model:
Momentum:
Induction:
Normalization
Discretization
Diagnostics
The following scalars are tracked during simulation:
- Perturbed kinetic energy:
en_U - Perturbed magnetic energy:
en_B - Background magnetic energy:
en_B_eq - Total magnetic energy including background:
en_B_tot - Perturbation total energy:
en_tot - Total energy including background contribution:
en_tot2
Examples

Standing shear-Alfvén wave
A single transverse velocity mode splits into two counter-propagating Alfvén waves, i.e. a standing wave. Its energy oscillates between the kinetic and the magnetic channel at twice the wave frequency, while the structure-preserving discretization keeps the sum constant. The launch condition is in a periodic interval of length , with and .

Shear-Alfvén wave dispersion
Excite a broadband transverse velocity perturbation and recover the shear-Alfvén dispersion relation ω = v_A k with Struphy’s linearized MHD solver. Both transverse velocity components are seeded with coefficient-noise amplitude . The background is so the reference Alfvén speed is .