Fig. 8: Effects of the normalized cross helicity.
From: Energy transfer of imbalanced Alfvénic turbulence in the heliosphere
A on the spectral index of \({{{{{\rm{\delta }}}}}}{{{{{{\bf{Z}}}}}}}^{{{{{{\boldsymbol{\pm }}}}}}}\) and B on the ratio between the energy transfer due to large-scale interactions (\({\varepsilon }_{{{{{{\rm{LS}}}}}}}\)) and the energy transfer due to local-scale interactions (\({\varepsilon }_{{{{{{\rm{local}}}}}}}\)) of \({{{{{\rm{\delta }}}}}}{{{{{{\bf{Z}}}}}}}^{{{{{{\boldsymbol{\pm }}}}}}}\). In A, the star symbols represent results from Shi et al.34, the upper and lower dotted-dashed lines indicate the spectral indices of \({{{{{\rm{\delta }}}}}}{{{{{{\bf{Z}}}}}}}^{\pm }\) being −1.00 and −1.67, respectively.
