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A Computational Study of Soot Formation in Methane Air Co-Flow Diffusion Flame Under Microgravity Conditions

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Abstract

An in-house developed code has been used to predict soot formation in a methane air co flow diffusion flame at normal gravity and at lower gravity levels of 0.5 G, and 0.0001 G (microgravity). There is an augmentation of soot formation at lower gravity levels because of lower buoyancy induced acceleration leading to an increased residence time. The peak temperature at microgravity is reduced by about 50 K than that at normal gravity level. The axial velocity under normal gravity and reduced gravity show negative values (relatively small in magnitude) near the wall at axial height beyond 15 cm; but axial velocity is never negative in microgravity condition. Peak value of soot volume fraction at 0.5 G and microgravity multiplies by a factor of ∼3 and ∼7, respectively of that at normal gravity. The zone of peak soot volume fraction shifts away from the axis towards the wings, as gravity level is lowered. In comparison to soot volume fraction, the factors of amplification of soot number density at reduced gravity and at microgravity are comparatively lower at 1.2 and 1.5 of that at normal gravity respectively. On the other hand, mean soot particle sizes at reduced gravity and microgravity increase to 1.5 and 2 times of that at normal gravity respectively.

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Authors and Affiliations

  1. Department of Mechanical Engineering, Heritage Institute of Technology, East Kolkata, India

    Arup Jyoti Bhowal

  2. Department of Mechanical Engineering, Indian Institute of Engineering Science and Technology, Shibpur, West Bengal, India

    Bijan Kumar Mandal

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  1. Arup Jyoti Bhowal
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  2. Bijan Kumar Mandal
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Correspondence to Arup Jyoti Bhowal.

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Bhowal, A.J., Mandal, B.K. A Computational Study of Soot Formation in Methane Air Co-Flow Diffusion Flame Under Microgravity Conditions. Microgravity Sci. Technol. 28, 395–412 (2016). https://doi.org/10.1007/s12217-016-9489-6

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  • DOI: https://doi.org/10.1007/s12217-016-9489-6

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