Lars Steffens, Ali Gülhan

DOI Number XXX-YYY-ZZZ

Conference Number HiSST-2022-318

To gather information about both particle and gas phase temperatures inside a scaled solid rocket
motor plume UV-VIS emission spectroscopy (UVVIS) and infrared emission spectroscopy (FTIR) have
been used. Additionally, a position resolving two-color pyrometer technique in the visible spectrum
range (Alumina Emission Measurements, AEM) has been developed to obtain a particle temperature
distribution of the whole plume. These three methods have been applied during the ESA-EMAP project
tests inside DLR’s VMK facility of scaled solid rocket motor plumes [1]. This project pursued activities
regarding the experimental modeling of alumina particulates in solid boosters (EMAP).
The UVVIS emission spectroscopy can be used to monitor the grey body radiation of the particle phase.
This allows determining the particle phase temperature. FTIR spectroscopy allows the identification of
gaseous species inside the plume such as CO2, CO, HCL and H2O. The emission lines of HCl can be used
to determine the gas phase temperature of the plume. Both methods thus monitor the radiation
intensity and the temperature over time at a certain position downstream the nozzle exit during the
propellant combustion process. The AEM consists of two optical cameras which have been equipped
with 10nm width optical bandpass filters to obtain intensity maps at two distinct wavelengths. The ratio
of these intensity maps can be evaluated into a temperature distribution of the plume.

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