SLiM: Semi-spectral Linear MHD Code

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SLiM: A Code for the Simulation of Wave Propagation through an Inhomogeneous, Magnetised Solar Atmosphere

Post by owlice » Tue May 10, 2011 7:59 am

SLiM: A Code for the Simulation of Wave Propagation through an Inhomogeneous, Magnetised Solar Atmosphere

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
http://adsabs.harvard.edu/abs/2007AN....328..313C

Bibcode: 2011ascl.soft05004C

Preferred citation method: Please contact schunker [at] mps.mpg.de for the appropriate acknowledgement

ID: ascl:1105.004
Last edited by Ada Coda on Tue Jul 24, 2018 10:02 pm, edited 1 time in total.
Reason: Updated code entry.
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