Independent identifiability of the weak-shock transition coefficient
Determine whether the weak-shock transition coefficient can be constrained independently of the cylindrical blast-wave source normalization in period-based infrasound analyses of hypersonic atmospheric entries.
References
It does not establish whether can be constrained independently of the source normalization, which remains a separate parameter-identifiability question.
The 39 observation points establish a strong monotonic trend (Spearman = −0.84, < 0.001), but the physical cause of this structure cannot be uniquely identified from this dataset alone. Along the single OSIRIS-REx entry trajectory, altitude, velocity, Mach number, ambient density, pressure, and deceleration co-vary systematically. As a result, the observations cannot determine whether the trend is primarily controlled by Mach number, atmospheric density, source altitude, changing aerodynamic coupling, emission-point assignment, or some combination of these factors.
Future work should extend these calibrations to additional controlled reentries, space-debris events, and well-observed bolides to determine which aspects of,, and are source-class specific and which reflect more general cylindrical blast-wave behavior.