Abstract: The semi-spectral linear MHD (SLiM) code follows the interaction of linear waves through an inhomogeneous three-dimensional solar atmosphere. The background model allows almost arbitrary perturbations of density, temperature, sound speed as well as magnetic and velocity fields. The code is useful in understanding the helioseismic signatures of various solar features, including sunspots.
Credit: Cameron, R.; Gizon, L.; Daiffallah, K.
Site: http://www2.mps.mpg.de/projects/seismo/ ... /SLiM.html
Preferred citation method: Please contact schunker [at] mps.mpg.de for the appropriate acknowledgement