All Tables

Table 1: Total wave energy fluxes $F_{\rm tors}$ (erg/ cm² s) generated as torsional waves in a single magnetic flux tube embedded in the solar convection zone are compared to the fluxes for transverse tube waves, $F_{\rm trans}$ and longitudinal tube waves, $F_{\rm long}$ ; note that the factor 4 (see discussion below Eq. (23)) was included in the computation of the wave energy fluxes for transverse tube waves. All presented fluxes were computed by using analytical methods only.