HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. In this paper we present an analysis of the performance of HARMONI’s SCAO system, based on a pyramid wavefront sensor operating in the I band. The impact of the telescope environment is examined, including windshake, primary mirror aberrations, and the dynamics and control of the ELT correctors (M4/M5). Optimisation of the control basis based on knowledge of the stress response of M4 is presented and the performance of secondary loops are analysed, including a low order loop for NCPA correction. Finally, a full end-to-end simulation of the HARMONI SCAO system is presented and compared with original error budgets.
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