“…For the latter one, two EMA approaches, namely the Maxwell-Garnett and Bruggemann models [20,21], are implemented, which allows for the tuning for the melting layer, depending on the melting state and the particle morphology [9]. For detailed descriptions of the EMVORADO (e.g., equations for simulating reflectivity and radial wind), readers are referred to [5]. In order to validate the impacts of LHN schemes, VISOP and RTTOV are [22] additionally used to provide synthetic satellite data.…”