Application of the Transient Finite Energy Method to Spacecraft Structures for Shock Environment Predictions
| dc.contributor.author | O'Donnell, Daniel Emory | en |
| dc.contributor.committeechair | Kapania, Rakesh K. | en |
| dc.contributor.committeemember | Philen, Michael Keith | en |
| dc.contributor.committeemember | Stoumbos, Tom James | en |
| dc.contributor.department | Aerospace and Ocean Engineering | en |
| dc.date.accessioned | 2026-06-11T08:00:22Z | en |
| dc.date.available | 2026-06-11T08:00:22Z | en |
| dc.date.issued | 2026-06-10 | en |
| dc.description.abstract | The modern spacecraft will encounter multiple mechanical shock events over the course of its mission, from the modest but repetitive jolts of ground transportation to the extreme accelerations produced by pyrotechnic devices during stage separation and deployment. These transient shock events have the potential to damage sensitive hardware and degrade functional performance, making it necessary to accurately characterize and predict the shock environment at critical locations throughout the structure. This research investigates the application of the Transient Finite Energy (TFE) method to predict shock response at remote structural locations resulting from a known Shock Response Spectrum (SRS) source specification. The TFE method operates across the SRS, time, and frequency domains, using a Finite Element Model (FEM) coupled with frequency-domain force recovery to transform an SRS source specification into physically meaningful forcing functions that preserve the temporal and spectral content discarded by conventional SRS-based methods. The TFE method takes advantage of the fact that an infinite number of time histories can satisfy a specified SRS. By applying many forcing functions with unique properties, a mean SRS response may be computed. The central physical premise is that each shock event imparts a finite impulse, a finite quantity of momentum transferred in a brief time window, even though the amplitude, rise time, and duration of individual events are statistical in nature. This finite-energy constraint lends the method its name and provides a bound on the recovered forces. Analytical capability for predicting shock environments using the TFE method has shown promise; however, the workflow introduces a chain of modeling decisions whose individual and combined influence on prediction quality must be understood before results can be trusted. This work seeks to make those assumptions explicit by examining the fundamentals of the TFE workflow and applying the method to a validated cantilever beam model to predict the shock environment at a remote response location and evaluate how the structural dynamics reshape the transmitted shock. | en |
| dc.description.abstractgeneral | Every spacecraft endures a series of violent jolts throughout its journey from the factory floor to orbit. Some are mild, like the bumps of a truck ride to the launch pad, while others are extreme, like the explosive charges that separate rocket stages during flight. These sudden bursts of energy can travel through the spacecraft's structure and damage delicate instruments, electronics, and optical systems. Engineers need to predict where and how severe these shocks will be long before the hardware is built and tested, but the tools traditionally used to describe shock environments reduce complex events down to a single curve that throws away important information about how the shock actually moves through a structure. This research develops and examines a method called the Transient Finite Energy (TFE) method, which pairs a computer model of a structure with a description of the shock at its source to predict what the shock will look like at other locations. Unlike conventional approaches, this method preserves the detailed timing and frequency content of the shock as it travels, capturing how the structure itself filters, amplifies, or dampens the energy along the way. The method is applied to a simple beam structure to predict the shock environment at a remote location and to demonstrate how the structure's own vibration characteristics reshape the shock as it propagates. | en |
| dc.description.degree | Master of Science | en |
| dc.format.medium | ETD | en |
| dc.identifier.other | vt_gsexam:47068 | en |
| dc.identifier.uri | https://hdl.handle.net/10919/143339 | en |
| dc.language.iso | en | en |
| dc.publisher | Virginia Tech | en |
| dc.rights | In Copyright | en |
| dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | en |
| dc.subject | Shock | en |
| dc.subject | Spacecraft Structures | en |
| dc.subject | Environment Predictions | en |
| dc.title | Application of the Transient Finite Energy Method to Spacecraft Structures for Shock Environment Predictions | en |
| dc.type | Thesis | en |
| thesis.degree.discipline | Aerospace Engineering | en |
| thesis.degree.grantor | Virginia Polytechnic Institute and State University | en |
| thesis.degree.level | masters | en |
| thesis.degree.name | Master of Science | en |
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