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Survey of Blunt Body Dynamic Stability in Supersonic Flow

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pressure fields and shockwaves could possibly excite dynamic <strong>in</strong>stabilities, there exists a clear means through which<br />

the specific heat ratio could modify dynamic stability.<br />

Krum<strong>in</strong>s [48] quantified this effect by compar<strong>in</strong>g the damp<strong>in</strong>g measured <strong>in</strong> air ( = 1.4) and Tetrafluoromethane<br />

(CF 4 , = 1.12) for bodies with sphere cone, spherical section, and tension shell forebodies. Shadowgraph images <strong>of</strong><br />

the tension shell <strong>in</strong> Fig. 29 exhibit drastically modified<br />

shock structure with the change <strong>in</strong> test gas. For the<br />

sphere cone, tests <strong>in</strong> air revealed a stabiliz<strong>in</strong>g damp<strong>in</strong>g<br />

coefficient while tests <strong>in</strong> CF 4 found the same<br />

configuration to be dynamically unstable. This po<strong>in</strong>ts to<br />

the composition <strong>of</strong> the medium as a possible reason for<br />

the higher than predicted oscillation growth that has<br />

been observed on missions such as Mars Pathf<strong>in</strong>der [54].<br />

Given the exploration <strong>in</strong>terest <strong>in</strong> bodies such as Mars<br />

and the potential implications <strong>of</strong> under predict<strong>in</strong>g<br />

damp<strong>in</strong>g by test<strong>in</strong>g <strong>in</strong> ground facilities utiliz<strong>in</strong>g air,<br />

further understand<strong>in</strong>g <strong>of</strong> this phenomena and<br />

development <strong>of</strong> facilities with variable test gas<br />

capabilities may benefit the community greatly.<br />

Figure 29. Shockwave shapes for a tension shell <strong>in</strong><br />

CF 4 and air [48]<br />

VI.<br />

Physical Mechanisms<br />

Understand<strong>in</strong>g the possible physical mechanisms that govern the vehicle’s dynamic response would aid <strong>in</strong><br />

reduc<strong>in</strong>g uncerta<strong>in</strong>ty. As is po<strong>in</strong>ted out by Abe et al [67], descriptions <strong>of</strong> both the oscillation growth and the<br />

subsequent limit cycle behavior lack a fundamental understand<strong>in</strong>g. This section will highlight the few proposed<br />

explanations that exist <strong>in</strong> the literature and provide further <strong>in</strong>sight to the phenomenon <strong>of</strong> dynamic stability.<br />

A. Pitch<strong>in</strong>g Moment Hysteresis<br />

Early <strong>in</strong>vestigations <strong>of</strong> blunt body dynamics showed that a negative correlation existed between the trends <strong>of</strong> the<br />

static and dynamic stability coefficients. Beam and Hedstrom [8] noted that small changes <strong>in</strong> the static stability<br />

derivative ( ) corresponded to oppos<strong>in</strong>g changes <strong>in</strong> the pitch damp<strong>in</strong>g coefficient, (<br />

̇<br />

). This<br />

observation led to a theory that suggested the direction <strong>of</strong> the pitch<strong>in</strong>g motion causes nonl<strong>in</strong>earities <strong>in</strong> the pitch<strong>in</strong>g<br />

moment slope due to the f<strong>in</strong>ite time delay that exists between changes <strong>in</strong> pitch angle and subsequent changes <strong>in</strong> the<br />

pressure field over the body. This hysteresis effect has been cited by other studies seek<strong>in</strong>g to describe the<br />

mechanism beh<strong>in</strong>d dynamic stability. It has been concluded both experimentally [68] and numerically [19] that the<br />

Figure 30. Pressure variation with pitch<strong>in</strong>g motion (left) and correspond<strong>in</strong>g hysteresis <strong>in</strong> pitch<strong>in</strong>g moment<br />

(right) [19]<br />

22 <strong>of</strong> 27<br />

American Institute <strong>of</strong> Aeronautics and Astronautics

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