Extinction Dynamics with the Underlying Physics of Ammonia and Ammonia/Hydrogen Spherical Diffusion Flames in Micro-Gravitational Condition

  • KANG Yinhu ,
  • LIU Junkun ,
  • HUANG Xiaomei ,
  • WU Pengfei ,
  • JIANG Zhijing ,
  • ZHANG Jiuyi ,
  • LU Xiaofeng
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  • 1. Key Laboratory of Low-grade Energy Utilization Technologies and Systems, Chongqing University, Ministry of Education of China, Chongqing 400044, China 
    2. Chongqing Changan Automotive Software Technology Co., Ltd., Chongqing 401120, China 
    3. School of Civil Engineering, Chongqing University, Chongqing 400044, China 
    4. College of Mathematics and Statistics, Chongqing University, Chongqing 400044, China

Online published: 2025-09-01

Supported by

The present research was supported by the National Natural Science Foundation of China (Grant No. 22178032), the Natural Science Foundation of Chongqing (Grant No. CSTB2023NSCQ-MSX1045), and National Key Research and Development Program of China (Grant No. 2022YFB4004404).

Copyright

Science Press, Institute of Engineering Thermophysics, CAS and Springer-Verlag GmbH Germany, part of Springer Nature 2025

Abstract

The utilization of ammonia as an alternative fuel is of great significance in the carbon neutrality strategy. However, the ammonia flame extinction mechanism induced by growing oscillations with its cramped flammability range, sluggish propagation speed, and poor stability is still not studied in sufficient details. In this paper, the high-fidelity simulations with efficient continuation computation and detailed models are conducted to investigate the ammonia extinction dynamics as a function of hydrogen blending ratio, and to reveal the governing sub-processes in flame extinction and oscillation development. It is found that the extinction and onset of oscillatory instability in the ammonia/hydrogen spherical diffusion flame (SDF) derive from the interaction of competing chemistry with diffusive leakage losses. Chemical oscillations occurring at the maximum temperature iso-contour are primarily responsible for the near-limit flame oscillations. In the rich-side low-temperature region, although the local heat production is inappreciable, the strong diffusive losses with governing, adverse contributions to the ignition chemistry play a leading role in flame extinction. The reactions dominating the extinction limit are also important for the oscillation frequency; the reactions that help to extend the extinction limit also tend to increase the frequency, and vice versa. The extinction limit and frequency depend mainly on the major reactant diffusivities (including NH3, H2, and O2) and heat conduction, while the diffusivities of other radicals and products are fairly unimportant. Hydrogen addition could remarkably extend the steady-state and oscillatory extinction limits of ammonia SDFs, and reduce the oscillation frequency since the imaginary eigenvalue is depressed.

Cite this article

KANG Yinhu , LIU Junkun , HUANG Xiaomei , WU Pengfei , JIANG Zhijing , ZHANG Jiuyi , LU Xiaofeng . Extinction Dynamics with the Underlying Physics of Ammonia and Ammonia/Hydrogen Spherical Diffusion Flames in Micro-Gravitational Condition[J]. Journal of Thermal Science, 2025 , 34(5) : 1672 -1691 . DOI: 10.1007/s11630-025-2153-y

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