HYPERSONIC FLEXWINGS

AS

ULTRALIGHT

WAVERIDER VEHICLES

 A CONCEPTUAL STUDY

BY

GORDON J. ROSS

ASTRA Program

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NB - Green numbers within brackets refer to references.

Introduction

Since the early eighties, interest in the family of vehicles known as Waveriders has grown dramatically . Research conducted by universities, government agencies and amateur groups, has clarified areas of Waverider dynamics which had previously hindered development of the concept . In particular, the drag characteristics of the Waverider have now been established , and research into the nature of hypersonic flow at Mach 20 is under way .

Much of the new knowledge has been gained through the use of Computational Fluid Dynamics (CFD) . Using complex flow modelling programmes, it is now possible to design a Waverider by changing the geometric shape of the shockwave. (1)

These optimised designs possess a far greater degree of subtlety than any Waverider which predates the use of CFD . The sudden realisation of the Waverider's potential has accelerated the rate of development in the field of hypersonic research . The first orbital test of a Waverider payload may be only two or three years away, as non-civilian Waverider programmes proceed with new vigour. (2) Civilian programmes will undoubtedly follow close behind, but unlike the defence researchers, civilian investigators have opportunities to design Waveriders for many applications.

One of the applications currently under study , is Aero-Gravity Assist (AGA). This technique entails utilising both the gravitational field of a planet, and its atmosphere, to effect major spatial course changes during interplanetary space flight. The concept is not a novel one, but the use of Waveriders for this purpose is new, and could significantly affect the range and costs of planetary exploration and development. With their high lift and low drag, Waveriders would permit large deflection angles, and in some cases, vector reversals, for vehicles on interplanetary trajectories.

It is partly for this reason that the Jet Propulsion Laboratory is looking at Waverider as a possible delivery system for their Solar Probe mission. (3) JPL is looking at the megasonic speed range, where velocities exceed Earth orbital speed, with planetary encounter speed of around Mach=100. The JPL Solar Probe mission requires a very high speed, high G manoeuvre in the atmospheres of both Venus and Mars, redirecting the orbital velocity of the Earth which the probe shared at launch and effectively cancelling it so that probe "falls" into a long elliptical orbit, whose perihelion lies within four solar radii, where it will measure the near-solar environment.

The design of Waverider vehicles for such a demanding mission poses many practical problems. The exact shape of a Mach=100 shockwave has to be determined, as well as the chemical interaction of gases encountering the shockwave at that velocity. It is fairly obvious that the Waverider for Mach=100 will have to be very slender indeed, and given the size and the mass of the Solar Probe payload (3) , this would require a very long vehicle, possibly too long to be flown in the Space Shuttle. This problem of size could make the entire vehicle impractical to build and perhaps impossible to launch.

Another problem area is attitude control. In its circuit, with the planet acting as a turning point, the spacecraft is in a forced orbit, flying upside down with aerodynamic lift directed towards the planet. The lift vector has to be reversed suddenly and with great precision in order to leave the atmosphere on the desired exit trajectory. In a previous paper (4) the author outlined a "conical roll" manoeuvre which inverted the vehicle while keeping the shockwave attached to the leading edges, and suggested "subtractive" control surfaces, described below, to bring about the manoeuvre.

The Solar Probe mission has spawned several types of Waverider AGA vehicles. Positioning of the payload in the airframe is critical to the stability of the configuration . (5) Although it has been suggested that the Waverider be built as part of the spacecraft solar heat shield, this would create the necessity for a detachable tail section. The problems of length to semispan ratio have led to a complete reappraisal of the concept of using Waveriders as interplanetary manoeuvring vehicle. The design of a multi-role Waverider for planetary exploration has long been an objective of researchers, and as such, the idea has some merit.

The difficulty up till now has been the seemingly insoluble problem of reducing the physical bulk of the Waverider to a packageable size. It is in this area that the solution has been found, from a rather unlikely source, which might make AGA and other Waverider applications a reality sooner than one might imagine.

The shape of optimised Waverider is not dissimilar to some form of low speed flexwing; in particular, there is a strong resemblance to early Rogallo delta wings. Both have delta planforms, both have highly swept wings, and both possess a double concavity in their lower surfaces. Townend, drawing on work by Penland,Daskin and Peldman, considered that the structure of a Waverider wing might be made partly flexible in order to save weight.(6)

Page Two

Hypersonic Flexwings Pages

Introduction
Part One
Part Two
Part Three
TERRESTRIAL HYPERSONIC FLEX-WING (THF)
INTERPLANETARY MEGASONIC FLEXWING (IMF)
AERODYNAMIC CONTROL AND MASS SHIFT
CONCLUSIONS
REFERENCES

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Website Author: Nick Portwin (portwin@easynet.co.uk)

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Date Last Modified: 31 07 1999