Polynyas, open water surrounded by sea-ice, are ubiquitous phenomena around Antarctica (Barber & Massom, 2007); they are sites of atmosphere-ocean heat exchange that create sea-ice (Morales Maqueda et al., 2004), and sea-ice produced in the coastal polynyas accounts for ∼10% of the Antarctic sea-ice cover (Tamura et al., 2008). The heat loss (open ocean polynyas, Wilson et al., 2019) and/or brine rejection resulting from the ice formation (coastal polynyas, Silvano et al., 2020) plays a key role in the generation of dense water, which contributes to Antarctic Bottom Water (AABW) and drives the global thermohaline circulation (Foldvik et al., 2004;Gordon et al., 2015;Ohshima et al., 2013;Williams et al., 2016). The increased ice production is thought to be the main reason for the recent recovery of AABW formation in the Ross Sea Polynya (RSP), for example, (Castagno et al., 2019;Silvano et al., 2020); therefore, observing sea-ice production (SIP) is crucial, as it can modify the Southern Ocean hydrography and alter the large-scale ocean circulation. We note that, in this article, the SIP can be positive (indicates ice growth) and negative (indicates melting).Polynyas can be classified into sensible-heat polynyas caused by the upwelling of warm water and latent-heat polynyas caused by sea-ice divergence due to offshore winds (Barber & Massom, 2007). Previous SIP research has primarily focused on latent-heat polynyas using the heat-budget (HB) method to estimate polynyas' SIP (e.g.,