Abstract A bow shock is generated by the interaction of solar wind with planetary global dipole field (e.g., Earth), or (mainly) ionosphere Mars). The cross‐shock potential has been well studied at Earth but not yet for Mars. We infer and approximate peak in frame invariant de Hoffmann‐Teller profile Mars ( ϕ ) data from Atmospheric Volatile EvolutioN (MAVEN) mission. find that its ratio to ram...