“…Measurements of VLF transmitter signals can be inverted to verify the theoretical ionospheric models (e.g., Bekker et al, 2022;Chowdhury et al, 2021) and remotely sense the electron density of D-region ionosphere (e.g., Gołkowski et al, 2018Gołkowski et al, , 2021Inan et al, 2010;Marshall et al, 2008;Xu et al, 2021), thereby investigating various space weather events, for example, solar flares (e.g., Han & Cummer, 2010;McRae & Thomson, 2004) and eclipses (e.g., Chakraborty et al, 2016;Cheng et al, 2023;Xu et al, 2019), and energetic particle precipitation from the radiation belts (e.g., Inan et al, 2007;Sauvaud et al, 2008). As for atmospheric processes, VLF measurements have been traditionally utilized to monitor lightning discharge (e.g., Bozóki et al, 2023;Qie et al, 2013) and thunderstorm activity (e.g., Kubisz et al, 2024;Qie et al, 2022). In addition, various high-energy radiation and transient luminous events in the Earth's atmosphere are associated with unique VLF signatures (Xu, Qie, et al, 2023;Yang et al, 2020;Zhang et al, 2020).…”