Infrared radiation signature of exhaust plume from solid propellants with different energy characteristics

Abstract The infrared radiation signature of the plume from solid propellants with different energy characteristics is not the same. Three kinds of double-base propellants of different energy characteristics are chosen to measure the infrared spectral radiance from 1000 cm −1 to 4500 cm −1 of their plumes. The radiative spectrum is obtained in the tests. The experimental results indicate that the infrared radiation of the plume is determined by the energy characteristics of the propellant. The radiative transfer calculation models of the exhaust plume for the solid propellants are established. By including the chemical reaction source term and the radiation source term into the energy equation, the plume field and the radiative transfer are solved in a coupled way. The calculated results are consistent with the experimental data, so the reliability of the models is confirmed. The temperature distribution and the extent of the afterburning of the plume are distinct for the propellants of different energy characteristics, therefore the plume radiation varies for different propellants. The temperature of the fluid cell in the plume will increase or decrease to some extent by the influence of the radiation term.

[1]  al e,et al.  Comparison of calculated and measured radiation from a rocket motor plume , 2001 .

[2]  Gang Li,et al.  The HITRAN 2008 molecular spectroscopic database , 2005 .

[3]  Jonathan M. Burt,et al.  Monte Carlo Simulation of Particle Radiation in High Altitude Solid Rocket Plumes , 2007 .

[4]  H. M. Shang,et al.  GRASP: A GENERAL RADIATION SIMULATION PROGRAM , 1997 .

[5]  S. Orszag,et al.  Renormalization group analysis of turbulence. I. Basic theory , 1986 .

[6]  A Monte Carlo Radiation Model for Simulating Rarefied Multiphase Plume Flows , 2005 .

[7]  Frederick S. Simmons,et al.  Rocket Exhaust Plume Phenomenology , 2000 .

[8]  S. Orszag,et al.  Renormalization group analysis of turbulence. I. Basic theory , 1986, Physical review letters.

[9]  S. Surzhikov Spectral and Narrow Band Directional Emissivity of Light-Scattering and Non-Scattering Volumes , 2002 .

[10]  M. Lev,et al.  Experimental and Computational Study of Infrared Emission from Underexpanded Rocket Exhaust Plumes , 2001 .

[11]  H. Pergament,et al.  Influence of Chemical Kinetic and Turbulent Transport Coefficients on Afterburning Rocket Plumes , 1971 .

[12]  N. Eisenreich,et al.  Radiation Emitted from Rocket Plumes , 1997 .

[13]  R. Reed,et al.  The standard infrared radiation model , 1981 .

[14]  Investigation of soot combustion in underexpanded jet plume flows , 2005 .

[15]  D. Jensen,et al.  Reaction rate coefficients for flame calculations , 1978 .

[16]  Stephen J. Young,et al.  Nonisothermal Band Model Theory , 1976 .

[17]  H. F. Nelson,et al.  Influence of particulates on infrared emission from tactical rocket exhausts , 1984 .

[18]  Direct simulation Monte-Carlo algorithms for the rocket exhaust plumes emissivity prediction , 2002 .

[19]  M. Modest Radiative heat transfer , 1993 .

[20]  H. F. Nelson Evaluation of rocket plume signature uncertainties , 1987 .

[21]  S. Surzhikov Monte Carlo Simulation of Plumes Spectral Emission , 2003 .