Visualisation of linear MHD waves in a coronal loop

Loop as a straight cylinder
A loop modeled as a straight cylinder

The theory of MHD waves in loops has been modeled by Edwin & Roberts (1983), where the loop is considered to be a straight cylinder with the equilibrium media inside and outside homogeneous. Across the interface, total pressure and radial displacement are continuous. The magnetic field is directed parallel to the cylinder axis.

To help understand how the linear MHD wave solutions look like, I have produced image and movies of the density perturbation and velocity, as well as dispersion diagrams for a typical coronal case (normalised w.r.t. internal sound speed):

CS,0 = 1.00, VA,0 = 2.00, CS,e = 0.50, VA,e = 5.00,
rhoe / rho0 = 0.2, Be / B0 = 1.00, Te / T0 = 0.25
beta0 = 0.30, betae = 0.01,

Dispersion diagrams

m=0 (sausage)

m=1 (kink)

m=2 (fluting or ballooning)

m=3 (fluting or ballooning)

m=4 (fluting or ballooning)

m=5 (fluting or ballooning)