Education
One axis holds the whole center together
Every facility, model and result in TEMPEST can be placed on a single logarithmic length scale. From left to right the axis spans 30 orders of magnitude. The center’s focus: in dynamic problems correlation’s impact propagates across these scales.
Interparticle spacing — molecular dynamics
Dust grain, Debye length — dusty plasma imaging
Kolmogorov scale — laboratory flows
Shock structure — blast chamber
Apparatus — tunnels and chambers
Boundary layer — atmosphere
Weather systems — planetary
Convection zone — stellar interiors
Supernova remnant — astrophysical
Interstellar medium — galactic
The dashed band marks the twelve decades TEMPEST reaches with hardware rather than inference. Inside it, a claim can be falsified directly. Outside it, on either end, the centre's job is to build models whose extrapolation can be trusted — and to say honestly how far that trust extends.
Five integrated areas
What the center actually does
1
Scale interactions
Turbulent flows couple every scale they contain, and no single model survives the whole range. This area builds machine-learned closures that pass information between molecular, continuum and astrophysical descriptions without breaking the conservation laws that hold them together.
2
Structure formation
Dusty plasmas are the rare turbulent system whose individual constituents can be imaged directly. Tracking every particle through the onset of collective motion gives the first direct observation of where a particle description hands off to a continuum one.
3
Transport mechanisms
In extreme parameter regimes the usual gradient-diffusion picture fails: transport at a point depends on conditions far away. Fractional-calculus and non-local formulations are developed and then tested against flows with viscosity ratios approaching 106.
4
Model validation
A prediction that cannot be falsified is not a prediction. This area builds the multi-scale validation framework — shared benchmarks, uncertainty budgets and data standards — that lets an experiment at one scale test a model built at another.
5
Cross-cutting technologies
Neural networks that quietly violate conservation of mass are worse than useless in a predictive setting. The centre develops structure-preserving architectures and tensor decompositions that hold conservation laws exactly while attacking the dimensionality that defeats conventional methods.
Explore the center
The five areas above are how the center is organized. They can be read in four ways: what we are trying to predict, where models lose the physics, how the science is actually done, and what comes out of it.
Mission
The TEMPEST mission
Three grand challenges make the need visible
Can fusion become a reliable source of energy? What determines whether a massive star explodes and spreads newly formed elements through the universe? How can a hypersonic vehicle or atmospheric-entry system be predicted before it is built or flown? These systems differ greatly, but each becomes uncertain when small-scale interactions that cannot be computed directly control a large-scale result.
Every useful model simplifies nature
Scientists move from particle interactions to statistical descriptions, from those descriptions to fluid-scale models, and from fluid motion to affordable models of turbulence and mixing. Each step makes prediction possible, but it also removes information. Scientists often call the rule that returns the influence of the removed information a closure. TEMPEST asks which missing influence truly matters and how it should be represented.
Studying one piece in isolation can hide the real source of error
A particle-scale model may be accurate while passing incomplete information to a fluid model. A fluid model may be accurate in a simple setting while failing when turbulence, shocks, material changes, or long-lived memory become important. An application code may then inherit errors created several modeling steps earlier. Looking at only one scale can improve a local piece without improving the final prediction.
This is why TEMPEST must be a Center
The needed connections cross plasma physics, fluid dynamics, applied mathematics, experiments, scientific computing, artificial intelligence, uncertainty analysis, national laboratories, and industry. A Center can align questions, measurements, simulation outputs, mathematical requirements, software, and workforce training across those boundaries. No single project, facility, or discipline can see the entire chain from microscopic interaction to application decision.
Fusion, supernovae, and hypersonics provide independent tests
TEMPEST does not assume that the three applications are the same. Their differences are scientifically valuable. A modeling idea that remains credible across distinct regimes is stronger evidence of captured physics than a model tuned to one experiment, one code, or one dataset. When an idea fails to transfer, the failure helps identify what information is still missing.
The science behind the mission
One connected chain of models
No practical calculation can resolve every particle, collision, chemical reaction, field, instability, shock, and turbulent structure. Scientists therefore use a sequence of models, each designed for a different scale. TEMPEST studies what is lost at each transition, when that loss changes the answer, and how the missing influence can be restored without making the calculation impossible.
Fusion energy: heat flow, stability, and mixing
A fusion plasma can be compressed and heated so quickly that particle motion, magnetic fields, material response, instabilities, and turbulent mixing all interact. TEMPEST asks which of these effects most strongly change energy gain, heat loss, magnetic-field evolution, mixing, and other design-relevant outcomes. Evidence can come from detailed particle simulations, controlled plasma and turbulence experiments, extreme-matter measurements, existing fusion data, and partner tests.
Supernovae and stardust: explosion, elements, and observable signals
A core-collapse supernova combines gravity, radiation, neutrinos, magnetic fields, nuclear matter, and turbulence. The same unresolved motions that influence whether the star explodes can also affect the production and mixing of elements and the signals observed by telescopes and detectors. TEMPEST connects models to shock motion, explosion energy, element production, neutrino signals, gravitational waves, and light.
Hypersonics: shocks, heating, and survivability
At extreme speed, shock waves interact with turbulent boundary layers, surface roughness, high-temperature chemistry, flow separation, and intense wall heating. TEMPEST asks what must be represented to predict forces, heat loads, separation, transition, performance, and safety before flight. Evidence comes from matched experiments and simulations, time-resolved measurements, and carefully designed comparisons.
A credible prediction needs more than a good fit
The model must obey basic physical rules, remain stable when used inside a simulation, produce physically meaningful states, agree with measurements that can distinguish competing explanations, and state how much uncertainty remains. A model that works only on the data used to build it is not enough.
The Center creates the missing connections
Experimental teams can measure effects that modelers need; theorists can state the rules a model must obey; AI researchers can represent relationships that are too complex for a simple formula; application teams can determine which errors actually matter. TEMPEST brings those roles into one repeated cycle of question, prediction, test, revision, and transfer.
Potential impacts
Better prediction changes how difficult science is pursued
Fusion experiments, large astronomical simulations, and hypersonic tests are expensive and cannot explore every possible condition. A trustworthy model does not replace measurement. It helps select the most informative experiment, interpret what was observed, identify the uncertainty that controls a decision, and show where new evidence is needed.
Energy
More reliable fusion models could help researchers choose experiments, compare design options, identify the transport or mixing processes that limit performance, and reduce uncertainty before costly hardware is built. The long-term opportunity is progress toward clean, firm energy and continued leadership in a strategically important technology.
Discovery
Supernovae are natural laboratories at scales no experiment can reproduce in full. Better models can connect simulations more rigorously to neutrino, gravitational-wave, and electromagnetic observations, clarify why some stars explode, and improve understanding of how elements are formed and dispersed as stardust.
Security and space
More trustworthy prediction of shocks, heat transfer, chemistry, separation, and instability could improve the interpretation of ground and flight tests, support safer atmospheric entry and access to space, and reduce reliance on trial-and-error development in high-consequence systems.
People and tools
TEMPEST will produce reusable datasets, software, benchmarks, documented models, uncertainty reports, experimental practices, and accessible explanations. It will also train scientists who can move among experiments, mathematics, computation, AI, software, and application needs.
A Center multiplies the value of each result
A dataset becomes more useful when several modeling teams use the same definitions and uncertainty information. A new method becomes more credible when independent experiments and applications test it. A trainee becomes more effective when they understand how their work connects to the larger scientific and national mission.
Hypotheses TEMPEST will test
The missing-information hypothesis
In many extreme systems, the main limitation is not simply that a computer grid is too coarse. Important interactions, particle distributions, memory, or small-scale structures have been removed when the model was simplified. Representing the right missing influence should improve prediction more than adding cost without changing the model itself.
The connected-scales hypothesis
Errors introduced at one modeling step can pass into the next. Particle-scale assumptions can change fluid transport; fluid-scale assumptions can change instability and mixing; turbulence assumptions can change an application outcome. Treating the steps together should identify failures that remain hidden when each piece is tested alone.
The physically guided AI hypothesis
AI can help learn complicated missing relationships from data, but the result will transfer more reliably when it is required to respect known physical rules, known limits, and uncertainty. Accuracy on one training dataset is not sufficient evidence.
The adaptive-model hypothesis
A single fixed model may be unnecessary in ordinary conditions and inadequate in extreme ones. A model that can recognize when additional information is needed—and add complexity only then—may provide a better balance of speed, accuracy, and reliability.
The discriminating-evidence hypothesis
Not all data are equally useful. Measurements and simulations designed to separate competing explanations should improve models faster than large collections of data that do not directly test the missing physics.
The transfer hypothesis
A scientific idea that improves prediction in fusion, supernovae, and hypersonic flow—or in carefully chosen parts of more than one application—has passed a stronger test than an idea tuned to one case. Failure to transfer is also valuable because it reveals the limits of the idea.
Evidence determines the next step
TEMPEST will use results to refine an idea, transfer it to a new setting, or stop investing in a path that is not supported. The purpose of a hypothesis is not to protect an expectation; it is to organize learning.
Questions that drive TEMPEST
What outcome must be predicted?
The question begins with a quantity that matters: fusion energy gain or mixing, supernova explosion energy or observable signals, hypersonic heat loads or vehicle performance. Starting with the outcome prevents the research from becoming disconnected from a real scientific or engineering need.
What may the model have left out?
The missing influence might be a particle interaction, a nonstandard distribution of particle speeds, a delayed response, transport across a large region, an instability, or unresolved turbulence. TEMPEST identifies the specific modeling step at which important information may have been removed.
What evidence can decide?
A useful test must distinguish between competing explanations. It may be a laboratory measurement, a high-detail simulation, an astronomical observation, a comparison across codes, or a partner benchmark. The evidence should be chosen because it can change our confidence, not simply because it is available.
What physical rules and uncertainty matter?
The proposed model must respect the rules required by the surrounding science, such as conservation of mass and energy, positive density and temperature, stable behavior, and correct results in well-understood limits. The remaining uncertainty must be stated clearly enough to support a decision.
What changes if the idea is right?
The result might alter an experiment, a simulation, a design choice, a measurement plan, a software module, or the decision to continue a line of research. This step turns a scientific question into a traceable path toward use.
The Center keeps the question complete
Application experts define the consequential outcome; experiments and observations provide decisive evidence; theory identifies the missing information and required rules; AI and computation provide flexible and efficient models; partners help determine whether the improvement changes practice.
How models simplify nature
From Particle Interactions to a Manageable Model
Why simplification is necessary
A real plasma or fluid contains an enormous number of interacting particles. Following every position, velocity, and collision over an application-sized region is far beyond practical computing. Scientists instead describe how particles are distributed and how groups of particles influence one another.
What can be lost
The average behavior may look simple even when correlations among particles, rare energetic particles, long travel distances, or delayed interactions control heat flow, diffusion, relaxation, or the formation of collective structures. Assuming those effects are unimportant can create an error before the model ever reaches the fluid scale.
What TEMPEST will do
The Center will combine detailed particle simulations, particle-resolved plasma experiments, extreme-matter measurements, and mathematical analysis to determine which interactions must be retained and which can be represented by a simpler rule.
How evidence will be used
Researchers will compare predicted transport, relaxation, distributions, and collective structures with measurements and high-detail calculations. The goal is not to reproduce every particle path; it is to reproduce the quantities that control the next level of prediction.
Why the connection to other scales matters
A particle-scale result is useful only if its influence can be carried into a fluid or application model. TEMPEST links the teams working at each step so the information passed forward is defined, tested, and usable.
From Particles to Fluid-Scale Models
Why fluid models are powerful
Instead of tracking every particle, a fluid-scale model follows a small set of average quantities across space and time. This makes it possible to simulate an entire fusion target, stellar region, or hypersonic flow.
Why averages may not be enough
Two particle populations can have the same density and temperature while carrying heat, stress, or directional motion in very different ways. Rapid compression, strong fields, shocks, or long travel distances can make those differences important.
How the missing influence can return
The model may need an additional quantity, a correction to heat or momentum transport, a history-dependent response, or a rule that activates only when the system leaves familiar conditions. TEMPEST will compare these options rather than assuming one formula works everywhere.
How TEMPEST will test the model
Detailed particle calculations and experiments will provide reference behavior. The reduced model will then be tested for accuracy, stable operation, physically meaningful states, and correct behavior when it returns to well-understood conditions.
Why a Center is needed
The variables chosen by particle and fluid researchers determine what turbulence and application teams receive. By designing this handoff together, the Center can avoid a common failure in which each individual model looks reasonable but the combined prediction does not.
Turbulence and Mixing
Why turbulence must be modeled
Turbulent motion spans a wide range of sizes. Resolving every motion in an application-scale calculation can be too expensive, so simulations compute the larger structures and model the influence of smaller ones.
Why extreme systems are harder
Standard approaches often assume that small-scale turbulence responds locally and quickly. Those assumptions can fail when shocks, strong material changes, particle trapping, rapidly growing instabilities, or long-lived structures create memory and transport over large distances.
What TEMPEST will measure
Shock facilities, variable-property flow experiments, instability and mixing experiments, particle tracking, velocity measurements, and high-detail simulations will reveal separation, transport, mixing, delayed response, and other quantities that a turbulence model must reproduce.
What TEMPEST will build
The Center will develop models that add memory, nonlocal influence, material changes, or learned corrections only when the evidence shows they are needed. The model must remain stable and affordable inside a large simulation.
Why the scales must stay connected
Turbulence is shaped by the fluid model it receives, and its effects feed directly into application outcomes. TEMPEST tests that full connection rather than validating a turbulence formula only in a separate, idealized flow.
How TEMPEST does the science
AI and Machine Learning
AI fills a defined gap
TEMPEST will not ask a black-box system to replace all of physics. Researchers first identify where a trusted model loses information, then use AI to represent the missing relationship, correction, or fast approximation.
Physical knowledge guides learning
A learned model can be required to conserve mass or energy, respect symmetry, keep density and temperature meaningful, remain stable, and recover known behavior in familiar limits. These requirements reduce the chance that a model fits one dataset while behaving unphysically elsewhere.
Uncertainty is part of the result
The model should indicate when it is being used outside the conditions supported by data. That information can guide a new experiment, a higher-detail simulation, or a decision to use a more complete model.
AI connects experiments and theory
Experiments reveal where current models fail; theory defines the rules and possible forms of the missing influence; AI provides a flexible representation; validation determines whether it transfers to new conditions.
Why a Center matters
Useful scientific AI requires coordinated data, physical expertise, software integration, validation, and application testing. TEMPEST brings those pieces together so a learned model is judged by scientific use, not only by a training score.
Theory and Modeling
Connecting scales is the central task
TEMPEST builds mathematical and computational bridges from particle interactions to statistical models, from statistical models to fluid behavior, and from fluid behavior to turbulence and application prediction.
Theory identifies the right variables
When a model fails, the answer may be another state variable, a delayed response, influence from a larger region, a better transport rule, or a recognition that the current modeling level is no longer adequate. Theory helps distinguish among these possibilities.
Credibility can be tested mathematically
Reduced and learned models should conserve the right quantities, remain stable, keep physical variables in meaningful ranges, and recover well-understood behavior when extreme effects disappear. These checks can rule out a model before it causes a failure in a large application simulation.
Simulation turns ideas into predictions
High-detail calculations create controlled reference cases; reduced calculations test speed and transfer; application simulations show whether the new model changes a consequential result.
The Center keeps theory connected to evidence and use
Mathematical ideas are developed with experimental measurements, AI representations, software requirements, and application questions in view. This helps prevent elegant theory from remaining detached from the quantities that can actually be tested.
Experiments and Data
Experiments are designed to answer model questions
The most useful measurement is not always the largest dataset. TEMPEST will identify observations that distinguish between competing explanations and show which modeling assumption needs to change.
The Center uses complementary platforms
Particle-resolved plasma experiments expose interactions and collective behavior. Shock and boundary-layer facilities reveal compression, separation, and memory. Variable-property and mixing experiments show how changing materials alter turbulence. X-ray measurements of extreme matter probe transport under conditions where ordinary assumptions may fail.
Controlled experiments isolate mechanisms
These facilities are not small copies of a complete fusion target, star, or vehicle. They create clean tests of specific processes so researchers can determine cause and effect, measure uncertainty, and compare models on common ground.
Shared evidence links the Center
Experimental teams, simulation teams, and application teams will agree on quantities, data formats, uncertainty descriptions, and comparison procedures. That allows a result from one platform to improve more than one model or application.
The loop continues
A measurement exposes a model failure; theory and AI propose an improved representation; simulation predicts a new signature; the next experiment tests that signature.
From research to impact
Education and Workforce
The science requires boundary-crossing skills
A researcher studying a missing modeling influence may need to understand how it is measured, how it enters an equation, how uncertainty is estimated, how software implements it, and why it matters to an application.
Training is built into the research
Cross-institutional exchanges, facility rotations, collaboration retreats, shared mentoring, interdisciplinary courses, and the TEMPEST Turbulence Symposium will place trainees inside teams that use different methods and language.
Communication and open science are core skills
Trainees will learn to document data and software, explain assumptions, create reproducible workflows, communicate with public and technical audiences, and understand how scientific evidence supports decisions.
The Center creates a network, not isolated apprenticeships
Students and postdoctoral researchers can connect universities, laboratories, industry, experiments, and application teams, carrying methods and questions across institutional boundaries.
Public Engagement and Access
Extreme science offers visible entry points
Fusion energy, exploding stars, hypersonics, turbulence, AI, and experiments can help people see how fundamental science connects to energy, discovery, security, space, and technology.
Accessible explanations build trust
Images, animations, plain-language pages, captions, alternative text, and clear statements of uncertainty can show what is known, what is being tested, and what TEMPEST expects to learn.
Participation must be broader than observation
Undergraduate research, community-college pathways, teacher resources, public programs, open educational material, and partnerships with under-resourced institutions can create routes into the work.
Open resources extend the Center
Where appropriate, datasets, software, benchmarks, tutorials, and public events will allow students, researchers, educators, and partners to reuse what TEMPEST creates.
Applications
Applications identify which errors matter
A modeling difference is important when it changes an outcome such as fusion gain, supernova explosion and element production, or hypersonic heat loads and performance. Application teams help the Center focus on quantities that can affect a scientific or engineering decision.
The three applications are independent tests
Fusion is a laboratory and design challenge, supernovae are observed cosmic events, and hypersonics combines ground tests, flight, chemistry, and fluid dynamics. An idea that transfers among them has survived very different evidence and operating conditions.
Validation proceeds in stages
TEMPEST first checks basic physical and mathematical behavior, then controlled simulations, then focused experiments or observations, then established application benchmarks, and finally partner-relevant use. Claims grow only as the evidence grows.
The applications feed back into fundamental science
A failed target calculation, a mismatch with an astronomical signal, or an inaccurate heat-load prediction can reveal which scale, measurement, or assumption needs attention.
A Center makes the comparison possible
Common definitions, shared data and software, coordinated uncertainty analysis, and cross-application teams allow the Center to distinguish a transferable scientific insight from a correction that works only in one setting.
Instruments you cannot get anywhere else
The experimental program is built around a handful of machines that reach conditions no other university group can produce, and around the decision to run them as one coordinated instrument.
| FACILITY | HOST | WHAT IT GIVES US |
|---|---|---|
| Variable-viscosity flow tunnel Viscosity ratios approaching 10⁶ | MSU | Multi-phase flows in which the working fluid changes character by six decades within one experiment. |
| Advanced Blast Chamber Largest university blast chamber | MSU | Shock–turbulence interaction with controlled, repeatable strong shocks. |
| Magnetized dusty plasma device Particle-resolved imaging | Auburn | Every constituent of the turbulent medium is individually visible and trackable. |
| Microwave-driven flow facility Volumetric energy deposition | MSU | Turbulence driven by absorbed electromagnetic energy rather than by boundaries. |
| OMEGA Laser Facility High-energy-density regimes | Rochester | Hydrodynamics at pressures and temperatures no table-top experiment reaches. |
Why this requires a center
The important connections cross scales, disciplines, facilities and applications
A single project can study one mechanism deeply. TEMPEST is designed to find out how those mechanisms connect — and whether an improvement at one scale actually strengthens the final prediction.
1
One chain of cause and effect
Particle interactions influence fluid transport; fluid behavior shapes instability and turbulence; turbulence changes application outcomes. Errors can move through the entire chain.
2
Evidence comes from different places
Experiments, detailed simulations, astronomical observations, and partner data each reveal a different part of the problem. Shared questions and measurements make the evidence connect.
3
Transfer is a stronger test
Fusion, supernovae, and hypersonics provide independent tests. An idea that survives across regimes is more trustworthy than one tuned to a single case.
4
People and tools must be shared
Cross-trained scientists, common software, documented data, coordinated facilities, and partner involvement allow insights to move instead of remaining isolated.
Models that keep their promises
A neural network that fits turbulence data beautifully while quietly losing mass is not a model, it is a curve. TEMPEST's cross-cutting programme develops structure-preserving architectures — networks whose conservation laws hold exactly by construction — together with tensor decompositions that make the dimensionality of the problem tractable.
The same commitment applies to validation. Every model released by the centre carries an uncertainty budget and a stated range of applicability on the scale axis above, and the data and code behind it are published openly.
Education
Education K-12
TEMPEST takes turbulence to the general public, through museum floors and community events across six states, as well as art, gaming, and digital media.
We want a research community that draws on the full range of human talent, and we build it by lowering the barriers between the public and the science.
Some of this work already runs in museums and at community events around the country. The rest is new: experiments in digital media, art, and games that will put turbulence in front of people who would never seek out a physics talk.
Three ways in
Turbulence in arts, games, and media
What happens when real flow physics become something you can watch, play, and paint.
Museums and community events
Seven sites, six states, and a microwave that makes plasma fireworks.
Removing barriers to entry
No coding to start, no special hardware, free or low-cost, and we go where the programs are missing.
Turbulence in arts, games, and media
We are launching a TEMPEST YouTube channel, built on team members whose science videos already reach wide audiences. A national art competition, open to the public, will connect creativity to multi-scale turbulence. A touring immersive exhibition will fill high-traffic halls with ceiling and wall projections that visitors can push and stir, so the physics becomes something they can touch.
We are exploring games that put players inside physically accurate turbulence, with partners such as MSU’s Games for Entertainment and Learning Lab, creators of the Quantum 3 mobile game on quantum physics. We are also exploring a game-engine plug-in bringing physically accurate turbulence to the gaming and film industries.
In virtual reality, a phone app built at Auburn already brings a virtual tokamak to outreach events, and it opens a family of phone and headset experiences for us to explore — for example plasma turbulence moving inside the virtual machine.
Museums and community events
We will coordinate our outreach with museums and community groups, including museums where TEMPEST members already run programs, such as the Rochester Museum and Science Center. We already use facilities like Science on a Sphere and a vortex demonstration that carries turbulence from planetary flows down to storms. At Rochester’s Science Alive, a scientist turns a microwave into a plasma firework: light at the kinetic level, sound at the fluid level, one phenomenon read at two scales at once.
Partner outreach programs already run at seven sites across six states, including STEM Fest at Baylor, Science on the Edge at Rochester, and Island Day at Texas A&M University–Corpus Christi. TEMPEST will coordinate these programs and expand their reach to thousands of students each year.
Removing barriers to entry
Our programs are designed to be free or low-cost. A phone, a browser, or a museum visit is enough to start.
- No coding background is needed to start, and the browser-based activities we build will run on ordinary hardware.
- We will direct outreach to under-resourced institutions and economically disadvantaged communities, where these programs are hardest to come by.
- For many students, community colleges are the main road into science. Programs such as the TARDIS Summer of Code bring computational research to community-college students across Michigan.
The breadth is deliberate. The portfolio covers activities such as museums, exhibitions, digital media, art, games, and community events. We will weigh each activity by its cost, impact, and risk, and expand the early pilots that work.
Opening the science itself
The MSU Turbulence Library is built for open access, so the data, codes, and teaching material the Center produces can be used far beyond it: a classroom, a company, a research group on another continent.
Most material will be openly licensed and will not require an affiliation with the Center. Trainees will add their own work to the library as part of their training, following open-science practice that keeps every dataset findable and reusable.
Get involved
To get involved with TEMPEST outreach, from hosting an event to partnering on a program, email Junlin Yuan at junlin@msu.edu.