AAWSAP DIRD, Detection and High-Resolution Tracking of Vehicles at Hypersonic Velocities, November 2010
DOW-UAP-D148 · page 23 of 46
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UNCLASSIFIED/fFOR. QFFIEl.t.L: Uii QD:I! X I x I06 i J \ \ I u(A, T 2) I ''!. \ \ SxI05 •. ! o~---~----~--------~---~ Figure 12. Energy Spectrum of the Sun at 5,778 K. Application of Planck's Law to Hypersonic Vehicles. As described in the theory of hypersonic fluid flow, any object moving through the atmosphere with an M > 1 will result in a shock wave emanating from the leading edge of the object. If the object has a blunt nose, such as a meteor entering the atmosphere, the shock will be detached from the surface. If we consider a spherical object moving through the atmosphere at hypersonic speed, as shown in Figure 13, the expected spectrum of emitted radiation can be computed. In this example, the altitude is assumed to be 10 km above the Earth's surface. At this altitude, the ambient static temperature is 223 K (- 50° C), the pressure is 26.1 % of sea level atmospheric pressure (see Appendix A for the properties of the U.S. Standard Atmosphere). UNCLASSIFIED//EQA: QlililEl.t.L: W&&: O,.L'l 19