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In previous work [1], three TAIJI orbital deployments have been proposed tocompose alternative LISA-TAIJI networks, TAIJIm (leading the Earth by$20^\circ$ and $-60^\circ$ inclined with respect to ecliptic plane), TAIJIp(leading the Earth by $20^\circ$ and $+60^\circ$ inclined), TAIJIc (colocatedand coplanar with LISA) with respect to the LISA mission (trailing the Earth by$20^\circ$ and $+60^\circ$ inclined). And the LISA-TAIJIm network has beenidentified as the most capable configuration for massive black hole binaryobservation. In this work, we examine the performance of three networks to thestochastic gravitational wave background (SGWB) especially for the comparisonof two eligible configurations, LISA-TAIJIm and LISA-TAIJIp. This investigationshows that the detectability of LISA-TAIJIm is competitive with the LISA-TAIJIpnetwork for some specific SGWB spectral shapes. And the capability ofLISA-TAIJIm is also identical to LISA-TAIJIp to separate the SGWB components bydetermining the parameters of signals. Considering the performances on SGWB andmassive black hole binaries observations, the TAIJIm could be recognized as anoptimal option to fulfill joint observations with LISA.

Alternative LISA-TAIJI networks: detectability of the isotropic stochastic gravitational wave background