Using Braginskij’s two-fluid description, the stability of the high m,n resistive ballooning mode is investigated under two interesting regimes typified by \(\omega_ s\ll | \omega | \leq \omega_ s/S\) and \(| \omega | \gg \omega_ s/S\) in the presence of classical resistivity, electron thermal conduction, and anomalous transport effects such as electron viscosity and radial thermal conductivity. It is assumed that the major contributions to the anomalous transport coefficients come either from the nonlinear terms \((\bar B.\nabla)P_ e\) and \((\bar B.\nabla)\chi_{\|}\) \((\bar B.{\bar \nabla})T_ e\), representing the parallel pressure gradient and thermal conduction terms, respectively, or from the microscopic turbulent fluctuations in density/temperature and magnetic field. A generalized set of coupled second-order equations in \({\bar \phi}\) and \({\bar \psi}\) is derived and solved to obtain analytical solutions by variational as well as asymptotic matching techniques. It is shown that the anomalous thermal transport term excites the new \(m=1\) resistive ballooning mode \((| \omega | \gg C_ s/qR)\) with a large growth rate. The excitation of the \(m=2\) type (or \(\Delta'\) driven) mode, on the other hand, is found to be strongly influenced by both anomalous electron viscosity and radial thermal conduction.