Supersonic jet mixing in the presence of two annular co-flow streams

Author:

S Rajkumar12,Vasanthakumar Parthasarathy2,Suseela Moorthi Aravindh Kumar1ORCID,Rathakrishnan Ethirajan3

Affiliation:

1. Department of Aerospace Engineering , SRM Institute of Science and Technology , Kattankulathur , Chengalpattu , Tamil Nadu , 603203 , India

2. School of Aeronautical Sciences , Hindustan Institute of Technology and Science , Padur , Chennai , Tamil Nadu , 603103 , India

3. Department of Aerospace Engineering , Indian Institute of Technology Kanpur , Kanpur , Uttar Pradesh , 208016 , India

Abstract

Abstract The mixing characteristics of a Mach 1.9 jet at three levels of overexpansion, corresponding to nozzle pressure ratio (NPR) 3, 4 and 5, in the presence of a sonic co-flow (secondary flow), which was submerged in a subsonic co-flow (tertiary flow) was studied experimentally. For these NPRs the secondary co-flow is sonic with underexpanded levels and the tertiary flow Mach number was found to be 0.41, 0.71 and 0.85, respectively. The centerline decay results of the primary jet show that the jet mixing is abated by the co-flow, at all levels of expansion. However, in spite of the reduced mixing encountered by the supersonic primary jet, the waves in the jet core are found to be weaker in the presence of co-flows. This may be regarded as an advantage from the shock associated noise point of view, in accordance with Tam’s theory; which states weaker the waves in the core, the lesser is the shock associated noise. The results show that the reduced mixing environment caused by the sonic co-flow alone leads to the jet core elongation of about 20%, 23% and 49%, at NPRs 3, 4 and 5, respectively. The core length of the jet is found to increase by 29%, 46% and 62%, respectively, at NPRs 3, 4 and 5, when both sonic and subsonic co-flow streams are present.

Publisher

Walter de Gruyter GmbH

Subject

Aerospace Engineering

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