1. Introduction
Liquid propellant rocket engines (LPREs) are a key technology for space launchers world wide. The liquid oxygen–hydrogen (LOX/H
) propellant combination offers the highest specific impulse among all flown chemical propellants.
1,2 The European Ariane 5 and Ariane 6 rely on LOX/H
rocket engines. Other recent examples include the Japanese LE-9,
3 the Russian RD-0146,
4 the Chinese YF-77,
5 and in the US, the RS-25 for the Space Launch System, the RL-10C, as well as the BE-3.
6 The liquid-oxygen/methane (LOX/CH
) combination is predicted to be cheaper and easier to handle than LOX/H
. Hence, there is growing interest in these propellants. Examples of LOX/CH
engines currently in development are the Japanese LE-8,
7 the Chinese TQ-11 and TQ-12, the European Prometheus
8 and M-10, as well as the Raptor and BE-4 in the US.
Due to its direct influence on flame anchoring, combustion stability, system pressure and overall performance, the injector design is a crucial element in the development of LPREs. The velocity ratio (
) and the momentum flux ratio (
) are non-dimensional numbers describing the shear forces from the velocity difference of the injected propellants and thus the atomisation and mixing. Therefore, they often serve as important design parameters governing the combustion efficiency of an engine.
9 Frequently, the injectors are placed in sub-scale experiments to verify the desired performance before implementing into full-scale engines.
10–19 These experiments can also provide test data to validate CFD tools for use in the design process.
Sub-scale experiments can also be used to assess the thermoacoustic stability characteristics of a particular injector design.
20,21 Thermoacoustic instabilities are caused by the coupling of oscillating heat release rate (
) with pressure oscillations (
) in the combustion chamber. Instabilities can arise if the Rayleigh criterion is satisfied, which can be expressed as
Measuring
at the wall of a combustion chamber is relatively straight forward, whereas
cannot be measured directly. In former studies, ultraviolet radiation measurements in the band corresponding to the hydroxyl radical (OH*) have often been used as a marker for heat release rate in sub-scale experiments.
22–24 The interpretation of such measurements can be complicated by the fact that OH* radiation suffers from high self-absorption at pressures relevant for most engines, resulting in the measured intensities dominated by the emission closest to the observer. Furthermore, at temperatures above 2700 K, OH* emission is dominated by thermal excitation rather than chemiluminescence preventing a direct relation between intensity and
. For highly strained flames, the peak temperature in the reaction zone is decreased and thus the latter effect is reduced.
25 In contrast, radiation in the blue wavelengths, for example, in the band corresponding to CH* emission, is considered to suffer less from the limitations affecting the OH* emission due to a higher ratio of excited to ground state concentrations for this radical. In addition, a shorter duration of the peak CH* concentration improves the suitability as markers for time-resolved heat release
26 under such conditions and can complement OH* measurements for the assessment of combustion dynamics.
14,24 Although lacking an established proportionality between line-of-sight integrated radiation measurements and
, the correlation of intensity with pressure can give a qualitative indication of the thermoacoustic interaction. Therefore, this article applies OH* and CH* radiation measurements as markers for heat release rate in rocket combustion at pressures well above the validated range. An assessment of the potential to use OH* and CH* emission as marker is performed by comparing the radiation measurements with the thermoacoustic state of the combustor.
A more straightforward approach to assessing the Rayleigh criterion is the direct extraction of
from simulations, which again emphasises the need for high-quality validation data. In addition to global parameters such as combustion chamber pressure and mass flow rates of oxidiser (
) and fuel (
), detailed information concerning flow parameters and boundary conditions are necessary to validate that the injection, atomisation, and combustion processes are captured correctly. Hence there is a need for suitable experimental data.
10,27 Here sub-scale combustion chambers play a special role since they can accommodate optical access and provide spatially resolved radiation measurements as a valuable point of comparison with numerical results.
The DLR optically accessible rocket combustor model ‘N’ (BKN) addresses the aforementioned need for validation test cases and enables multiple opportunities for validation. The experiment is extensively equipped with conventional diagnostics, such as thermocouples and pressure sensors and is, therefore, able to provide well-defined boundary conditions, which can be compared to steady-state simulations or time-averaged results of unsteady simulations. The same applies to the large optical access window enabling the examination of a great portion of the flame and providing information on the steady-state flame topology. A time-resolved comparison between experiment and unsteady simulations can be performed by comparing the acoustic amplitudes or sequences of flame snapshots, as well as via qualitative comparison of thermoacoustic interaction facilitated by the 2D Rayleigh Index distributions under different sets of operating conditions presented later in this article.
This work presents experiments with BKN and the propellant combination of LOX and compressed-/liquefied-natural-gas (CNG/LNG) and a comparison with previous experiments with the same injection element but hydrogen (H) as the fuel. In the tests with hydrocarbon fuel, high-speed imaging of OH* and CH* radiation was conducted. While there is no formation of CH* in LOX/H combustion, the same optical filter for CH* was used in the H tests to capture the blue radiation in the same wavelength range.
First, the experimental setup including the optical diagnostics and operating conditions will be presented for the latest experiments with LOX/CNG/LNG. Then, the methodology of the performed analysis will be described. The influence of four LOX/LNG operating conditions on the flame topology will be shown and discussed in comparison to previous LOX/CNG and LOX/H experiments. Finally, the flame response during intervals with high-amplitude, self-excited oscillation of the longitudinal acoustic resonance modes will be compared to intervals without significant excitation of the acoustic modes.
5. Conclusion
Four different operating conditions of thermoacoustically unstable and stable combustion in an experimental rocket combustor with large optical access using the propellant combination LOX/LNG were presented in detail in this work. The propellants were injected through a shear coaxial injection element. Simultaneous flame radiation imaging of the ultraviolet and blue wavelength ranges was conducted. In combination with the axial development of temperature and pressure signals, well-defined information on the boundary conditions in the combustion chamber is provided and allows the usage of this dataset as a test case for validating numerical modelling of LOX/methane flames.
Features characterising the flame topology were derived from the time-averaged imaging and compared to previous experiments with the oxidiser-fuel combinations of LOX/CNG and LOX/H. Here, the major influence of the longitudinal combustion instabilities on the flame opening angle and flame length were evident. While for unstable combustion the flame opening angle was significantly larger, the flame length was nearly half the length of previous more stable tests. This behaviour was also reflected in the hot gas and wall temperature measurements within the chamber. The hot gas temperature reached its peak between 100 and 150 mm downstream of the faceplate, corresponding to the end of the shortened flame, and then decreased towards the end of the chamber.
2D Rayleigh Index distributions were calculated using the acoustic field reconstructed from unsteady pressure measurements and the high-speed blue as well as ultraviolet radiation measurements. The distributions and integrated values reflect the observed state of thermoacoustic excitation of the chamber and shows the potential of OH* and especially CH* measurements as a qualitative marker for heat release rate. For the three unstable load points, a strong interaction between flame radiation intensity and acoustic pressure oscillations covering nearly the whole flame zone is determined. Comparison to previous experiments with the propellant combinations of LOX/CNG and LOX/H revealed consistent behaviour. Higher values of the integrated Rayleigh Index accompany higher normalised acoustic pressure amplitude. Integral Rayleigh Indices for the whole window area in dependence of frequency were also consistent with the thermoacoustic state of the chamber. If the Rayleigh criterion is satisfied, then the marker for heat release rate must be acceptable, at least within the uncertainty of phase. These data are hoped to serve the community in the validation of numerical tools for the prediction of combustion instability in LOX/LNG rocket engines.
The pressure bursts preceding the self-sustaining combustion instabilities in Test 2, in the literature referred to as intermittency,
38 could indicate the operation of the combustor under bi-stable conditions. The changed operating conditions could, therefore, lead to changed boundary conditions in the chamber supporting the transition to self-sustaining, high-amplitude combustion instabilities. The precise circumstances leading to stable, intermittent, or unstable combustion is the subject of the ongoing investigation.