solar interior $(\beta >>1)$. Hence, at the photospheric/chromospheric level, a transition layer exists where $\beta \sim 1$. The objective of the present work is to study the influence of the plasma $\beta$, in the range $[10^{-3},1]$, on the properties of the jet model of PAD09. By doing so, it is possible not only to study the validity of our jet model in the different layers of the solar atmosphere but also, at a given scale, to compare and possibly explain the various properties of jets observed in different environments, e.g., in coronal holes or active regions.

In the highly stratified solar atmosphere, jet-like events are expected to occur in a complex multi-$\beta$ environment. Numerous recent numerical models have thus simulated different jet-like events in a stratified atmosphere including a rich range of physical processes: spicules [e.g., @MartinezSykora11; @MartinezSykora13], chromospheric jets [e.g., @YangL13b], surges [@NobregaSivero16], and coronal jets [e.g., @MorenoInsertis13; @FangF14; @Torok16]. In this paper we complement these studies by performing simulations within a relatively uniform atmosphere, but with varying $\beta$. By simplifying the environment compared to the real solar atmosphere, we are able to isolate parametrically the role of the plasma $\beta$ parameter in a controlled way. This facilitates clearer 