Predicting Rocket Fuel Combustion Using Surrogate Models
Research on modeling combustion behavior in hybrid rockets for improved safety.
Georgios Georgalis, Alejandro Becerra, Kenneth Budzinski, Matthew McGurn, Danial Faghihi, Paul E. DesJardin, Abani Patra
― 6 min read
Table of Contents
- The Slab Burner and Its Importance
- Challenges in Predicting Combustion
- The Need for Uncertainty Quantification
- The Role of Surrogate Models
- Setting Up the Experiments
- Testing the Surrogates
- Propagating Uncertainty
- Calibration of Parameters
- Results and Discussions
- Future Work
- Conclusion
- Original Source
- Reference Links
In the world of rocket science, the need for precision is crucial. Imagine trying to launch a rocket while juggling flaming balls; even a tiny mistake could lead to a sizzling disaster. This paper focuses on understanding how to predict how a type of rocket fuel burns inside a 2D slab setup. This involves using computer simulations and fancy statistical tricks to account for uncertainties in the fuel's burning behavior.
The Slab Burner and Its Importance
A slab burner is a setup used in testing hybrid rockets, which combine solid and liquid fuels. Hybrid rockets have become popular because they offer the density of solid fuels with the controllability of liquids. Think of it as ordering a pizza with your favorite toppings while keeping the crust just right. Researchers experiment with various fuels like paraffin because they can ignite faster and create a better burn rate.
The burning process is complex because it involves a liquid layer forming on the solid fuel, which can lead to some very interesting combustion phenomena. When this happens, the fuel vapors escape and mix with the oxidizer, resulting in a combustible mixture.
Challenges in Predicting Combustion
Predicting how things will burn is not as easy as flipping a switch. Combustion involves many factors, including how gases flow, how they mix together, and how the heat affects the fuel. Each of these factors operates on different time and length scales, which makes it tricky. For instance, the chemical reactions happen quickly, while the gas flow takes its sweet time.
This multifaceted nature creates problems for scientists trying to simulate combustion accurately. They often need high-performance computing resources, similar to those used in video games, but, you know, much more complex.
Uncertainty Quantification
The Need forThe uncertainty in combustion predictions can lead to serious issues. This is where uncertainty quantification (UQ) steps in. UQ helps scientists figure out the effects of unknowns in their models. If you’ve ever prepared a meal without knowing if you have enough ingredients, you can appreciate how important it is to know the right quantities. UQ helps researchers decide how much they can trust their simulations.
Using UQ, researchers can start with the known variables of the reactions and the inputs that affect the outcome. By doing this, they can begin to understand what might go wrong before they light the match, so to speak.
Surrogate Models
The Role ofSince running simulations can take too long-imagine waiting 24 hours to see if your idea works-scientists create surrogate models. These models act like shortcuts-they’re easier and quicker to run while still giving valuable insights. Think of them as the 'fast track' line at an amusement park. Two types of surrogate models were tested in this study: Gaussian Processes (GP) and Hierarchical Multiscale Surrogates (HMS).
The GP model is like a friendly guide: it uses statistics to predict what outcomes might be based on previous data. HMS, on the other hand, is a bit more sophisticated; it looks at data at different scales to give a more nuanced view.
Setting Up the Experiments
To get started, the researchers used a combination of computer models and real-life experiments. They created 64 simulations through a process called Latin Hypercube Sampling-a method that sounds complicated but essentially ensures they’re testing a variety of scenarios.
Through these experiments, they gathered data on how different parameters-like the heat of sublimation (how much heat it takes to change from solid to gas)-affect combustion. They figured out which parameters really mattered for the predictions and which ones could be safely ignored.
Testing the Surrogates
The researchers trained both the GP and HMS models using the data collected from their simulations. They then compared how well each model predicted the combustion outcomes by using cross-validation. Cross-validation is a fancy way of saying they made sure their models worked by testing them on different sets of data.
Both models did well, but there were notable differences. The GP model showed some sensitivity to its settings, like a diva demanding the perfect lighting before taking the stage. Meanwhile, the HMS was more robust and handled the complexities of combustion more gracefully.
Propagating Uncertainty
Once the models were validated, the researchers used them to propagate the uncertainty from the inputs to the desired outcomes, specifically the regression rate-a measure of how quickly the fuel is consumed. This is the key to understanding how well the rocket will perform.
The results showed variations in the expected combustion rate in different regions of the burner. For example, the front part of the slab was where the action happened, while the middle was like a quiet lunch hour at a busy cafe.
Calibration of Parameters
To refine their models further, the researchers used a technique called Bayesian calibration. This method helps adjust their models based on real-world observations. They looked at how the fuel’s heat of sublimation and the temperature exponent in their chemical reactions compared with experimental results.
After performing this calibration, the researchers found that their earlier assumptions were slightly off. It turns out the values they initially used were not getting them the desired outcomes. With proper tuning, the models began to align better with the real-world data.
Results and Discussions
The main findings highlighted the effectiveness of both surrogate models in predicting fuel combustion behavior. They showed that both GP and HMS can perform well even in complex multiscale problems-something that’s quite an achievement in the rocket science world.
Moreover, the uncertainty propagation using the HMS model revealed important details regarding the burning rates in different regions. They observed a range of burn rates that could help inform future designs, making them safer and more efficient.
The calibration process showed its value as well, as it revealed the need for better-informed parameter estimates. These improved estimates led to better predictive performance, illustrating how essential it is to keep refining models with actual data.
Future Work
The journey doesn’t end here. The researchers plan to explore more sophisticated fuels and combustion scenarios to gain further insights. By investigating more options like higher alkanes or even different geometries, they can enhance their understanding of hybrid rocket systems.
Moreover, they’re keen on developing surrogates capable of estimating time-dependent combustion behavior. This is like having a GPS that not only tells you how to get to your destination but can also anticipate heavy traffic along the way.
Conclusion
In conclusion, this work provides valuable insights into the complexities of predicting combustion behaviors in hybrid rockets using state-of-the-art models. The rigorous UQ process, alongside the development of surrogate models, outlines a pathway for more reliable predictions in the future.
As researchers continue to refine these techniques and incorporate real-world data, the world of rocket science might just become a bit easier to navigate. And who knows-maybe one day, we'll be sending rockets to Mars without breaking a sweat!
Title: UQ of 2D Slab Burner DNS: Surrogates, Uncertainty Propagation, and Parameter Calibration
Abstract: The goal of this paper is to demonstrate and address challenges related to all aspects of performing a complete uncertainty quantification (UQ) analysis of a complicated physics-based simulation like a 2D slab burner direct numerical simulation (DNS). The UQ framework includes the development of data-driven surrogate models, propagation of parametric uncertainties to the fuel regression rate--the primary quantity of interest--and Bayesian calibration of critical parameters influencing the regression rate using experimental data. Specifically, the parameters calibrated include the latent heat of sublimation and a chemical reaction temperature exponent. Two surrogate models, a Gaussian Process (GP) and a Hierarchical Multiscale Surrogate (HMS) were constructed using an ensemble of 64 simulations generated via Latin Hypercube sampling. Both models exhibited comparable performance during cross-validation. However, the HMS was more stable due to its ability to handle multiscale effects, in contrast with the GP which was very sensitive to kernel choice. Analysis revealed that the surrogates do not accurately predict all spatial locations of the slab burner as-is. Subsequent Bayesian calibration of the physical parameters against experimental observations resulted in regression rate predictions that closer align with experimental observation in specific regions. This study highlights the importance of surrogate model selection and parameter calibration in quantifying uncertainty in predictions of fuel regression rates in complex combustion systems.
Authors: Georgios Georgalis, Alejandro Becerra, Kenneth Budzinski, Matthew McGurn, Danial Faghihi, Paul E. DesJardin, Abani Patra
Last Update: 2024-11-09 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.16693
Source PDF: https://arxiv.org/pdf/2411.16693
Licence: https://creativecommons.org/licenses/by/4.0/
Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.
Thank you to arxiv for use of its open access interoperability.