The Effect of Flow and Magnetic Twist on Resonant Absorption of Slow MHD Waves in Magnetic Flux Tubes

Observations show that there are twisted magnetic flux tubes and plasma flow throughout the solar atmosphere. The main purpose of this work is to obtain damping rate sausage modes in presence twist flow. We dispersion relation for slow continuity an inhomogeneous layer under conditions pores, then we solve it numerically. For selected density profile, field, as a function radius across layer, effect field on resonance absorption at low speed greater than one high speed.