FLIGHT MEASUREMENTS OF LOW-VELOCITY BOW SHOCK ULTRAVIOLET-RADIATION

被引:28
作者
ERDMAN, PW
ZIPF, EC
ESPY, P
HOWLETT, C
LEVIN, DA
LODA, R
COLLINS, RJ
CANDLER, GV
机构
[1] UNIV PITTSBURGH, DEPT PHYS & ASTRON, PITTSBURGH, PA 15260 USA
[2] UTAH STATE UNIV, DEPT PHYS, LOGAN, UT 84322 USA
[3] UTAH STATE UNIV, CTR SPACE ENGN, LOGAN, UT 84322 USA
[4] INST DEF ANAL, DIV SCI & TECHNOL, ALEXANDRIA, VA 22311 USA
[5] UNIV MINNESOTA, DEPT ELECT ENGN, MINNEAPOLIS, MN 55455 USA
[6] N CAROLINA STATE UNIV, DEPT MECH & AEROSP ENGN, RALEIGH, NC 27695 USA
关键词
Electron counter - Flowfield - Rocket nose payload - Ultraviolet sensors;
D O I
10.2514/3.11566
中图分类号
O414.1 [热力学];
学科分类号
摘要
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 (FST). 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.
引用
收藏
页码:37 / 41
页数:5
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  • [1] LEVIN DA, UNPUB J THERMOPHYSIC