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Propagation of fast-mode magnetohydrodynamic (MHD) compression waves istraced in the Galactic Center with a poloidal magnetic cylinder. MHD wavesejected from the nucleus are reflected and guided along the magnetic field,exhibiting vertically stretched fronts. The radio threads and non-thermalfilaments are explained as due to tangential views of the waves driven bysporadic activity in Sgr A$^*$, or by multiple supernovae. In the latter case,the threads could be extremely deformed relics of old SNRs exploded in thenucleus.

Galactic Centre Threads as Nuclear MHD Waves