Abstract

This study focuses on the development of two analytical models that describe the wall-bounded cyclonic flowfield in a hemispherical domain. The closed-form solutions that we pursue are motivated by the need to characterize the swirling bidirectional motion engendered in an upper stage thrust chamber, namely, the VR35K-A VORTEX® engine, conceived and developed by Sierra Nevada Corporation. Our analysis proceeds from the Bragg–Hawthorne formulation, which is quite effective in the treatment of steady, inviscid, and axisymmetric flows. In this work, we show that two rotational solutions may be derived for particular specifications of the stagnation head and tangential angular momentum expressions that appear in the Bragg–Hawthorne equation. Then, with the parental streamfunctions in hand, other properties of interest are deduced and these include the main velocity and pressure variations, vorticities, crossflow velocities, extensional and shearing strain rates, virtual energy dissipation rates, and both axial and polar mantle distributions; the latter consist of pairs of rotating, non-translating interfacial layers, separating the so-called inner and outer bidirectional and bipolar regions, respectively. More specifically, two Beltramian solutions are identified with mantles that appear at 50% and 61.06% of the chamber radius, respectively. By matching the outlet radius of the chamber to the mantle location in the equatorial plane, the outflow is permitted to exit the chamber seamlessly. In both models, the axial and radial velocities vary linearly with the injection speed and a characteristic inflow parameter consisting of a geometric ratio of the inlet area and the chamber radius squared.

Highlights

  • Theoretical models of wall-bounded cyclonic flowfields continue to receive attention in the fluid dynamics and propulsion communities due to their direct relevance to a variety of swirl-augmented combustion devices and novel thrust chambers for engines under development

  • We show that two rotational solutions may be derived for particular specifications of the stagnation head and tangential angular momentum expressions that appear in the Bragg–Hawthorne equation

  • Two mathematical formulations are pursued as viable alternatives to describe the bulk cyclonic motion inside a hemispherical enclosure

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Summary

INTRODUCTION

Theoretical models of wall-bounded cyclonic flowfields continue to receive attention in the fluid dynamics and propulsion communities due to their direct relevance to a variety of swirl-augmented combustion devices and novel thrust chambers for engines under development. Besides the inviscid assumption underlying most of the ensuing models, their outcomes have been rather effective at identifying several distinct classes of cyclonic flow profiles, namely, the quasi complex-lamellar, Beltramian, generalized Beltramian, and Trkalian types.35 In addition to these developments, the incorporation of a hollow core in a cyclonic chamber has been pursued by Barber et al., where the backflow generated in the downdraft is accounted for. When uniform injection is paired with inviscid and adiabatic conditions, the flow becomes homentropic and the Bragg–Hawthorne equation reduces to a linear function of the tangential angular momentum This enables us to derive a set of rotational profiles of the Beltramian helical type.

PROBLEM FORMULATION
Fundamental assumptions
Geometric configuration
Bragg–Hawthorne equation
Streamfunction representation and boundary conditions
Normalized variables and boundary conditions
BELTRAMIAN SOLUTIONS
Bidirectional and bipolar inner and outer regions
Axial and polar velocities and mantles
Type-0 case
Type-1 case
Bidirectional and bipolar zonal analysis
Radial velocity analysis
Pressure distribution
Vorticity distribution
Virtual dissipation and principal strain rates
Findings
CONCLUSIONS
Full Text
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