Flight measurements of low-velocity bow shock ultraviolet radiation

The ultraviolet spectrum, atomic oxygen 130.4-nm radiation intensity, total plasma density, and electron temperature of a Mach 12 bow shock were obtained by a sounding rocket experiment launched from the Wallops Flight Facility (WFF) on April 25, 1990 at 12:32 a.m. Eastern Standard Time (EST). A two...

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Veröffentlicht in:Journal of thermophysics and heat transfer 1993-01, Vol.7 (1), p.37-41
Hauptverfasser: Erdman, Peter W, Zipf, Edward C, Espy, Patrick, Howlett, Carl, Levin, Deborah A, Loda, Richard, Collins, Robert J, Candler, Graham V
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Sprache:eng
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Zusammenfassung:The ultraviolet spectrum, atomic oxygen 130.4-nm radiation intensity, total plasma density, and electron temperature of a Mach 12 bow shock were obtained by a sounding rocket experiment launched from the Wallops Flight Facility (WFF) on April 25, 1990 at 12:32 a.m. Eastern Standard Time (EST). A two-stage, Terrier Malamute rocket which attained an apogee of 720 km was used in this experiment. Optical data in the 200-400-nm wavelength range were obtained from 37 to 75 km at a vehicle velocity of 3.5 km/s at various locations on the 0.1016-m radius hemispherical dome. Electron probe and VUV OI 130.4-nm, measurements were obtained near nose cone ejection at 37 km. This article presents a discussion of the instruments used and the key data obtained.
ISSN:0887-8722
1533-6808
DOI:10.2514/3.11566