Overview

Localized heat leaks in cryogenic fuel systems can trigger boil-off, tank over-pressurization, and long-duration mission failure. This project uses acoustic accelerometer data and unsupervised machine learning to identify distinct boiling regimes, translating raw vibration signals into physically interpretable cluster groupings that can inform future space fuel management systems.

446
Runs
36
Features
6
Regimes
99%
Stability
73%
Rand Index

Team: Hailey Ernest, Colin Hassett, Elliot Kunz, Cameron Hafer  ·  Advisors: Dr. Kelly Bodwin, Dr. Alex Dekhtyar  ·  Cal Poly SLO · Statistics, Mathematics, Computer Science

Methodology

Feature Engineering: 36 features engineered from time and frequency domains, designed to capture signal structure rather than raw amplitude. Detrending removes runtime-correlated drift; pairwise cross-accelerometer features capture differences between both sensors, a correction to prior work that used only one.

Dimensionality Reduction: PCA, diffusion maps, and UMAP were evaluated head-to-head. UMAP produced the clearest separation and was selected for the final pipeline.

Clustering: K-Means, HDBSCAN, and spectral clustering were compared. HDBSCAN was chosen for its ability to handle variable-density clusters and naturally identify outliers. Final pipeline: UMAP + HDBSCAN.

Results: Six Boiling Regimes

  • Lack of Boiling: filtered by noise-floor threshold before clustering
  • Sporadic: rare, isolated spikes with no consistent timing
  • Chaotic: irregular bursts of varying height and frequency
  • Rhythmic: consistent, repeating spike patterns
  • Dense / Double Rhythmic: distinct subclusters within rhythmic boiling
  • Single Rhythmic with Climax: rhythmic behavior with a distinctive amplitude peak
UMAP + HDBSCAN Main Clusters

UMAP + HDBSCAN: three active boiling clusters

Rhythmic Subclusters UMAP

Subclustering within the rhythmic regime

Research Poster

NASA Capstone Poster

Full Report

Navigate the 13-page final report below.

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