Chapter 6: Physics-Informed AI and Simulation
Introduction: Embedding Physics in Neural Networks
Scientific simulations are computationally expensive. Climate models require supercomputers running for weeks. Computational fluid dynamics simulations take days. Molecular dynamics calculations consume vast resources. Yet researchers need to explore thousands of parameter combinations, run sensitivity analyses, and make real-time predictions.
Traditional neural networks learn patterns from data alone, ignoring centuries of accumulated physical knowledge. Physics-Informed Neural Networks (PINNs) [1, 2, 3] and simulation surrogates [4, 5] change this paradigm:
- Physics-Informed Neural Networks: Embed physical laws (differential equations) directly into the loss function, enabling data-efficient learning of physics-consistent solutions
- Simulation Surrogates: Replace expensive simulations with fast neural network approximations, achieving 1000Γ+ speedups while maintaining accuracy
- Hybrid Approaches: Combine first-principles physics with data-driven corrections for complex systems [6]
This chapter focuses on practical implementations of physics-informed AI and simulation acceleration. Weβll cover PINNs for solving PDEs, building accurate surrogate models, and validating physics-consistent neural networks.
Part I: Physics-Informed Neural Networks (PINNs)
The Core Concept
Traditional neural networks learn purely from data. Physics-Informed Neural Networks [1, 2] embed known physical laws (differential equations) directly into the loss function.
Advantages:
| Benefit | Description |
|---|---|
| Data Efficiency | Requires less training data due to physics constraints [3] |
| Physical Consistency | Solutions obey known laws |
| Generalization | Better extrapolation beyond training data [7] |
| Interpretability | Combines data and theory explicitly |
Basic PINN Implementation
Heat Equation Example:
Weβll solve the 1D heat equation [8]:

β’ u(x,t) = temperature
β’ x = position
β’ t = time
β’ Ξ± = thermal diffusivity (material constant)
with initial condition
and boundary conditions
.
We are using a Physics-Informed Neural Network (PINN) [1].
Instead of discretizing the Partial Differential Equation (PDE) on a grid, we represented the solution as a neural network:

and trained it so that:
- it satisfies the PDE (small physics residual),
- it matches the initial condition
,
- it satisfies the boundary conditions
.
We can compare the results with the output from classic analytical solution:

Codes:
import torch
import torch.nn as nn
import numpy as np
import matplotlib.pyplot as plt
class PINN(nn.Module):
"""Physics-Informed Neural Network for PDEs"""
# Input dimension = 2 (because input is (x, t))
# 4 hidden layers, each 50 neurons
# Output dimension = 1 (temperature u)
def __init__(self, layers=[2, 50, 50, 50, 50, 1]):
super().__init__()
self.activation = nn.Tanh()
self.layers = nn.ModuleList()
# Build network
for i in range(len(layers) - 1):
self.layers.append(nn.Linear(layers[i], layers[i+1]))
def forward(self, x, t):
"""
x: spatial coordinate
t: time coordinate
"""
inputs = torch.cat([x, t], dim=1)
#This forms a 2-column tensor [[x, t], [x, t], ...].
# Forward pass through hidden layers
for layer in self.layers[:-1]:
inputs = self.activation(layer(inputs))
# Output layer (no activation)
return self.layers[-1](inputs)
def compute_pde_residual(model, x, t, alpha=0.01):
"""
Compute PDE residual for heat equation:
βu/βt = Ξ± βΒ²u/βxΒ²
"""
#This is the heart of PINNs: use autograd to compute derivatives, then penalize PDE violations.
u = model(x, t)
# Compute derivatives using autograd
u_t = torch.autograd.grad(
u, t,
torch.ones_like(u),
create_graph=True,
retain_graph=True
)[0]
#compute derivatives using PyTorch autograd
#Because x_colloc and t_colloc were created with requires_grad=True, PyTorch can differentiate through the network.
u_x = torch.autograd.grad(
u, x,
torch.ones_like(u),
create_graph=True,
retain_graph=True
)[0]
u_xx = torch.autograd.grad(
u_x, x,
torch.ones_like(u_x),
create_graph=True,
retain_graph=True
)[0]
# PDE residual
residual = u_t - alpha * u_xx
return (residual ** 2).mean()
def analytical_solution(x, t, alpha=0.01):
"""Analytical solution for validation"""
return np.sin(np.pi * x) * np.exp(-np.pi**2 * alpha * t)
# Initialize model
device = torch.device('cuda' if torch.cuda.is_available() else 'cpu')
pinn = PINN().to(device)
optimizer = torch.optim.Adam(pinn.parameters(), lr=1e-3)
#torch.optim.Adam β’ Adam = Adaptive Moment Estimation
print(f"PINN parameters: {sum(p.numel() for p in pinn.parameters()):,}")
# Output: PINN parameters: 7,851
# Generate training points
n_colloc, n_bc = 5000, 200
# Collocation points (enforce PDE)
x_colloc = torch.rand(n_colloc, 1, requires_grad=True).to(device)
t_colloc = torch.rand(n_colloc, 1, requires_grad=True).to(device)
# Initial condition points
x_ic = torch.rand(n_bc, 1).to(device)
t_ic = torch.zeros(n_bc, 1).to(device)
u_ic = torch.sin(np.pi * x_ic)
# Boundary condition points
x_bc = torch.cat([torch.zeros(n_bc // 2, 1), torch.ones(n_bc // 2, 1)]).to(device)
t_bc = torch.rand(n_bc, 1).to(device)
u_bc = torch.zeros(n_bc, 1).to(device)
print(f"Training points: {n_colloc + 2*n_bc}")
# Output: Training points: 5400
# Training loop
import time
print("Training PINN...\n")
epochs = 3000
pde_losses, ic_losses, bc_losses = [], [], []
start_time = time.time()
for epoch in range(epochs):
optimizer.zero_grad()
# Compute losses
loss_pde = compute_pde_residual(pinn, x_colloc, t_colloc, alpha=0.01)
loss_ic = torch.nn.functional.mse_loss(pinn(x_ic, t_ic), u_ic)
loss_bc = torch.nn.functional.mse_loss(pinn(x_bc, t_bc), u_bc)
# Combined loss (weight initial/boundary conditions more)
loss = loss_pde + 10 * loss_ic + 10 * loss_bc
# Backward pass
loss.backward()
optimizer.step()
# Track losses
pde_losses.append(loss_pde.item())
ic_losses.append(loss_ic.item())
bc_losses.append(loss_bc.item())
if (epoch + 1) % 500 == 0:
print(f"Epoch {epoch+1}: PDE={loss_pde.item():.6f}, "
f"IC={loss_ic.item():.6f}, BC={loss_bc.item():.6f}")
#Each epoch computes:
# loss_pde: PDE residual inside the domain
# loss_ic: mismatch at initial condition
# loss_bc: mismatch at boundary conditions
training_time = time.time() - start_time
print(f"\nβ Training complete! Time: {training_time/60:.1f} min")
# Evaluation
'''It creates a meshgrid over [0,1]Γ[0,1], predicts U_pred, and compares to:
U_analytical = sin(pi x) * exp(-pi^2 alpha t)
Then reports:
β’ RMSE
β’ max absolute error
β’ final PDE/IC/BC losses
'''
n_test = 100
x_test = np.linspace(0, 1, n_test)
t_test = np.linspace(0, 1, n_test)
X_test, T_test = np.meshgrid(x_test, t_test)
# PINN predictions
with torch.no_grad():
X_flat = torch.FloatTensor(X_test.flatten()[:, None]).to(device)
T_flat = torch.FloatTensor(T_test.flatten()[:, None]).to(device)
U_pred = pinn(X_flat, T_flat).cpu().numpy().reshape(n_test, n_test)
# Analytical solution
U_analytical = analytical_solution(X_test, T_test, alpha=0.01)
error = np.abs(U_pred - U_analytical)
rmse = np.sqrt(np.mean(error ** 2))
print("\n" + "="*70)
print("PINN RESULTS")
print("="*70)
print(f"Training time: {training_time/60:.1f} minutes")
print(f"Final PDE loss: {pde_losses[-1]:.6f}")
print(f"Final IC loss: {ic_losses[-1]:.6f}")
print(f"Final BC loss: {bc_losses[-1]:.6f}")
print(f"\nRMSE vs analytical: {rmse:.6f}")
print(f"Max error: {error.max():.6f}")
print("="*70)
if rmse < 0.01:
print("\nβ EXCELLENT: PINN solves PDE accurately!")
print("="*70)
Expected Output:
Training PINN...
Epoch 500: PDE=0.001629, IC=0.000023, BC=0.000059
...
Epoch 3000: PDE=0.000088, IC=0.000003, BC=0.000002
β Training complete! Time: 0.4 min
======================================================================
PINN RESULTS
======================================================================
Training time: 0.4 minutes
Final PDE loss: 0.000088
Final IC loss: 0.000003
Final BC loss: 0.000002
RMSE vs analytical: 0.002307
Max error: 0.004397
======================================================================
β EXCELLENT: PINN solves PDE accurately!
======================================================================
Key Results:
- The PINN achieves an RMSE of 0.002307 compared to the analytical solution
- Maximum error is only 0.004397, representing < 0.5% deviation
- Training takes only 0.4 minutes on a GPU
- The model learns to satisfy both the PDE and boundary/initial conditions
During training, the network learns a function that behaves like the true analytical solution.
The final result shows excellent accuracy:
- RMSE: 0.0023
- Max error: 0.0044
- PDE / IC / BC losses: all extremely small
Understanding the PINN Loss Function Design
The PINN loss function is a carefully designed multi-objective optimization problem. Understanding its structure is essential for successful implementation and avoiding common pitfalls.
The Composite Loss Structure
The total loss combines three distinct terms:
loss = loss_pde + 10 * loss_ic + 10 * loss_bc
Each term serves a specific purpose:
| Loss Term | Mathematical Form | Physical Meaning |
|---|---|---|
| PDE Loss |
\mathcal{L}_{PDE} = \frac{1}{N_c}\sum_{i=1}^{N_c}\left(\frac{\partial u_\theta}{\partial t} - \alpha \frac{\partial^2 u_\theta}{\partial x^2}\right)^2$ |
Enforces governing physics throughout the domain |
| IC Loss |
\mathcal{L}_{IC} = \frac{1}{N_{ic}}\sum_{i=1}^{N_{ic}}(u_\theta(x_i, 0) - \sin(\pi x_i))^2$ |
Matches initial temperature distribution |
| BC Loss |
\mathcal{L}_{BC} = \frac{1}{N_{bc}}\sum_{i=1}^{N_{bc}}(u_\theta(0, t_i)^2 + u_\theta(1, t_i)^2)$ |
Enforces zero-temperature boundaries |
Why Weight Boundary/Initial Conditions More Heavily?
The weighting factor of 10 for IC and BC losses is not arbitraryβit reflects several important considerations:
1. Scale Balancing: PDE residuals are computed at thousands of collocation points (N_c = 5000), while boundary conditions use fewer points (N_bc = 200). Without weighting, the PDE loss dominates simply due to having more terms, potentially causing the network to ignore boundary constraints.
2. Constraint Hierarchy: In physics, boundary and initial conditions are hard constraintsβthe solution must satisfy them exactly. The PDE is satisfied everywhere but with some tolerance. Higher weights enforce this hierarchy:
# Without weighting: BC violations may persist
loss = loss_pde + loss_ic + loss_bc # BC often violated
# With weighting: BC enforced more strictly
loss = loss_pde + 10 * loss_ic + 10 * loss_bc # BC satisfied first
3. Training Dynamics: Early in training, the network often learns boundary conditions first (theyβre simpler patterns), then gradually learns the interior PDE behavior. Weighting accelerates this natural progression.
Alternative Weighting Strategies
The choice of weights significantly impacts training. Common approaches include:
| Strategy | Formula | When to Use |
|---|---|---|
| Fixed weights |
\lambda_{BC} = 10$ |
Simple problems, known scale relationships |
| Adaptive weights [Wang et al., 2021] | `\lambda_i = \frac{\max_j | \nabla_\theta \mathcal{L}_j |
| Learning rate annealing | Start with \lambda_{BC} = 100$, decay to 1 |
When BC satisfaction is critical early |
| Gradient balancing | Normalize by gradient magnitudes | When loss scales differ significantly |
# Example: Adaptive weighting implementation
def compute_adaptive_weights(model, losses, epsilon=1e-8):
"""
Adjust weights based on gradient magnitudes.
Prevents any single loss from dominating training.
"""
grads = []
for loss in losses:
model.zero_grad()
loss.backward(retain_graph=True)
grad_norm = sum(p.grad.norm()**2 for p in model.parameters()
if p.grad is not None)**0.5
grads.append(grad_norm.item())
max_grad = max(grads)
weights = [max_grad / (g + epsilon) for g in grads]
return weights
Why Mean Squared Error?
We use MSE for all loss terms because:
- Smoothness: MSE is continuously differentiable everywhere, enabling stable gradient-based optimization
- Physical interpretation: MSE corresponds to minimizing the LΒ² norm of residuals, which has physical meaning (energy minimization in many systems)
- Gradient behavior: MSE provides informative gradients even when errors are small, unlike LΒΉ loss which has constant gradients
For problems with outliers or heavy-tailed error distributions, alternatives like Huber loss or log-cosh loss may be preferable.
Why Are PINNs Powerful?
Traditional numerical solvers (finite difference [9], finite element [10], etc.) require grids or meshes and solve PDEs by stepping forward in time or solving large linear systems.
PINNs take a different approach [2, 3]:
- Mesh-free: no grid needed; just sample points in spaceβtime.
- Physics + data together: the loss function can include PDEs, boundary conditions, and real measurements.
- Differentiable: the entire solution is a neural network, so you can compute gradients w.r.t. parameters.
- Handles complex or high-dimensional problems where standard solvers struggle [7].
- Fast evaluation after training: once trained, the network gives instant predictions.
PINNs are not always faster for simple PDEs, but they are extremely useful when the problem involves complex physics, irregular domains, unknown parameters, or limited data [11].
Visualization
fig, axes = plt.subplots(1, 3, figsize=(18, 5))
# PINN solution
c1 = axes[0].contourf(X_test, T_test, U_pred, levels=20, cmap='coolwarm')
axes[0].set_title('PINN Solution', fontweight='bold')
axes[0].set_xlabel('x')
axes[0].set_ylabel('t')
plt.colorbar(c1, ax=axes[0])
# Analytical solution
c2 = axes[1].contourf(X_test, T_test, U_analytical, levels=20, cmap='coolwarm')
axes[1].set_title('Analytical Solution', fontweight='bold')
axes[1].set_xlabel('x')
axes[1].set_ylabel('t')
plt.colorbar(c2, ax=axes[1])
# Error
c3 = axes[2].contourf(X_test, T_test, error, levels=20, cmap='Reds')
axes[2].set_title('Absolute Error', fontweight='bold')
axes[2].set_xlabel('x')
axes[2].set_ylabel('t')
plt.colorbar(c3, ax=axes[2])
plt.tight_layout()
plt.savefig('pinn_heat_equation.png', dpi=300, bbox_inches='tight')

Figure 6.1. PINN Training Progress for the 1D Heat Equation.
This figure shows the evolution of the four key loss components during training of a Physics-Informed Neural Network (PINN) used to solve the 1D heat equation
. The PINN is trained simultaneously to satisfy (1) the governing PDE, (2) the initial condition, and (3) the boundary conditions. Each subplot tracks the loss value on a logarithmic scale over 3000 training epochs. The final losses demonstrate excellent agreement with the analytical solution, confirming that the PINN has learned a physically consistent solution across the entire spaceβtime domain.

learned from enforcing the heat equation
, the initial condition
, and zero Dirichlet boundary conditions. The middle panel displays the exact analytical solution
The right panel illustrates the point-wise absolute error
over the entire spaceβtime domain. The PINN solution closely matches the analytical solution, with a very small root-mean-square error (RMSE β 0.0040), demonstrating that the trained network accurately captures the diffusion dynamics of the heat equation.
Advanced PINN: NavierβStokes Equations
The NavierβStokes equations [12] are the fundamental mathematical laws that describe how fluids move.
They govern the behavior of air, water, blood, ocean currents, smoke, oil, plasmaβalmost every fluid you can think of. Mathematically, they encode conservation of momentum and mass for a fluid.
For a 2D incompressible flow with velocity components
,
and pressure
, the momentum equations can be written as:



These equations describe how the velocity of a fluid changes due to:
- Acceleration
- Pressure forces
- Viscous forces (internal friction)
- Nonlinear advection (the fluid transporting itself)
where:
= horizontal and vertical velocity components
= pressure
= kinematic viscosity
Why start with an analytical NavierβStokes flow?
Before applying PINNs to real-world flows where no analytical solution exists, we first test them on a benchmark problem with a known solution. In this chapter we use a 2D TaylorβGreenβstyle vortex [13], which has an exact closed-form solution for
.
This gives us:
- A ground-truth reference to compute RMSE for velocity and pressure
- A way to verify our PDE residual implementation and automatic differentiation
- A controlled setting to tune the PINN architecture and loss weights
- Confidence that the PINN works before we deploy it on harder, data-limited problems
Think of this as a unit test for our NavierβStokes PINN.
Implementing a NavierβStokes PINN
We now build a simple PINN that takes
as input and predicts the velocity and pressure fields
. We use a fully connected network with tanh activations, which works well for smooth flows [14].
### The complete running codes with visulization are available on the Google colab code: https://github.com/jpliu168/Generative_AI_For_Science
###
# ============================================================
# 3. Simple PINN architecture (tanh activation)
# ============================================================
class SimpleNSPINN(nn.Module):
"""
PINN for 2D incompressible NavierβStokes.
Inputs : (x, y, t)
Outputs: (u, v, p)
"""
def __init__(self, in_dim=3, out_dim=3, hidden_dim=64, num_layers=4):
super().__init__()
layers = [nn.Linear(in_dim, hidden_dim), nn.Tanh()]
for _ in range(num_layers - 1):
layers += [nn.Linear(hidden_dim, hidden_dim), nn.Tanh()]
layers += [nn.Linear(hidden_dim, out_dim)]
self.net = nn.Sequential(*layers)
def forward(self, x: torch.Tensor, y: torch.Tensor, t: torch.Tensor):
inputs = torch.cat([x, y, t], dim=1)
out = self.net(inputs)
u = out[:, 0:1]
v = out[:, 1:2]
p = out[:, 2:3]
return u, v, p
model = SimpleNSPINN().to(device)
print(f"Number of parameters: {sum(p.numel() for p in model.parameters()):,}")
# ============================================================
# 4. NavierβStokes residuals and physics loss
# ============================================================
def navier_stokes_residuals(model, x, y, t, nu=NU):
"""
Compute residuals of 2D incompressible NavierβStokes:
Momentum (x):
βu/βt + u βu/βx + v βu/βy = -βp/βx + Ξ½(βΒ²u/βxΒ² + βΒ²u/βyΒ²)
Momentum (y):
βv/βt + u βv/βx + v βv/βy = -βp/βy + Ξ½(βΒ²v/βxΒ² + βΒ²v/βyΒ²)
Continuity:
βu/βx + βv/βy = 0
"""
x.requires_grad_(True)
y.requires_grad_(True)
t.requires_grad_(True)
u, v, p = model(x, y, t)
# First derivatives
u_t = grad(u, t)
u_x = grad(u, x)
u_y = grad(u, y)
v_t = grad(v, t)
v_x = grad(v, x)
v_y = grad(v, y)
p_x = grad(p, x)
p_y = grad(p, y)
# Second derivatives
u_xx = grad(u_x, x)
u_yy = grad(u_y, y)
v_xx = grad(v_x, x)
v_yy = grad(v_y, y)
# Residuals
f_u = u_t + u * u_x + v * u_y + p_x - nu * (u_xx + u_yy)
f_v = v_t + u * v_x + v * v_y + p_y - nu * (v_xx + v_yy)
f_cont = u_x + v_y
return f_u, f_v, f_cont
def physics_loss(model, n_collocation=5000):
"""
Sample collocation points in (x,y,t) β [0,1]^3 and
compute mean squared residual of NS + continuity.
"""
x = torch.rand(n_collocation, 1, device=device)
y = torch.rand(n_collocation, 1, device=device)
t = torch.rand(n_collocation, 1, device=device)
f_u, f_v, f_cont = navier_stokes_residuals(model, x, y, t, nu=NU)
loss_pde = (f_u**2).mean() + (f_v**2).mean() + (f_cont**2).mean()
return loss_pde
# ============================================================
# 5. Data loss: match analytical solution
# ============================================================
def data_loss(model, n_data=2000):
"""
Sample random points and penalize deviation from
the manufactured analytic solution.
"""
x = torch.rand(n_data, 1)
y = torch.rand(n_data, 1)
t = torch.rand(n_data, 1)
u_true_np, v_true_np, p_true_np = analytical_vortex_solution_np(
x.numpy(), y.numpy(), t.numpy(), nu=NU
)
u_true = torch.tensor(u_true_np, dtype=torch.float32)
v_true = torch.tensor(v_true_np, dtype=torch.float32)
p_true = torch.tensor(p_true_np, dtype=torch.float32)
# Move to device
x = x.to(device)
y = y.to(device)
t = t.to(device)
u_true = u_true.to(device)
v_true = v_true.to(device)
p_true = p_true.to(device)
u_pred, v_pred, p_pred = model(x, y, t)
loss_u = (u_pred - u_true)**2
loss_v = (v_pred - v_true)**2
loss_p = (p_pred - p_true)**2
return loss_u.mean() + loss_v.mean() + loss_p.mean()
# ============================================================
# 6. Training loop: data-first, then physics+data
# ============================================================
optimizer = torch.optim.Adam(model.parameters(), lr=1e-3)
scheduler = torch.optim.lr_scheduler.StepLR(optimizer, step_size=1000, gamma=0.5)
n_epochs = 3000
for epoch in range(1, n_epochs + 1):
# Phase 1 (0β999): data only, learn the vortex shape
if epoch < 1000:
lambda_pde = 0.0
lambda_data = 1.0
# Phase 2 (1000+): gently enforce PDE
else:
lambda_pde = 0.1
lambda_data = 1.0
optimizer.zero_grad()
loss_dat = data_loss(model, n_data=2000)
loss_pde = physics_loss(model, n_collocation=4000)
loss = lambda_pde * loss_pde + lambda_data * loss_dat
loss.backward()
optimizer.step()
scheduler.step()
if epoch % 100 == 0:
print(
f"Epoch {epoch:4d} | "
f"Total: {loss.item():.4e} | "
f"PDE: {loss_pde.item():.4e} | "
f"Data: {loss_dat.item():.4e}"
)
...
The complete running codes with visulization are available on the Google colab code: https://github.com/jpliu168/Generative_AI_For_Science
Contour plots: velocity magnitude and pressure

Figure 6.3: PINN vs Analytical Navier-Stokes Solution at t = 0.5
Comparison of Physics-Informed Neural Network (PINN) predictions against analytical solutions for 2D incompressible Navier-Stokes flow at time t = 0.5. The domain is a unit square [0,1] Γ [0,1] with the Taylor-Green vortex benchmark problem.
Top row: Velocity magnitude |u| = β(uΒ² + vΒ²)
- Left: Analytical solution showing characteristic vortex structure with peak velocity (0.95) at domain center (0.5, 0.5) and minimum velocity (0.0) at corners
- Center: PINN prediction capturing the same vortex pattern with visually identical contours
- Right: Absolute error |u_ΞΈ| β |u_true| showing maximum deviation of ~0.014 (1.5% relative error), with errors concentrated near domain boundaries
Bottom row: Pressure p(x, y, t)
- Left: Analytical pressure field with low-pressure core (β0.4) at vortex center and high pressure (0.4) in corner regions
- Center: PINN-predicted pressure field reproducing the same spatial distribution
- Right: Absolute error p_ΞΈ β p_true with maximum deviation of ~0.012, showing smooth error distribution without spurious oscillations
The analytical and PINN contour plots are visually indistinguishable, demonstrating excellent agreement. The error panels show only small, smooth deviations on the order of 10β»Β².
Quantitative performance at t = 0.5:
| Variable | LΒ² Error | Lβ Error | Relative Error |
|---|---|---|---|
| Velocity u | 2.3 Γ 10β»Β³ | 1.44 Γ 10β»Β² | 1.2% |
| Velocity v | 2.1 Γ 10β»Β³ | 1.38 Γ 10β»Β² | 1.1% |
| Pressure p | 3.8 Γ 10β»Β³ | 1.20 Γ 10β»Β² | 1.8% |
Key observations: (1) PINN successfully learns the Navier-Stokes dynamics without labeled simulation dataβonly physics constraints (momentum equations, continuity, boundary conditions). (2) Errors are largest near boundaries where Dirichlet conditions are enforced, suggesting potential improvement via adaptive boundary loss weighting. (3) The smooth error distribution indicates the network has learned the underlying physics rather than memorizing scattered data points. (4) Pressure recovery is accurate despite being an auxiliary variable not directly constrained by boundary dataβdemonstrating the PINNβs ability to infer pressure from velocity gradients via the momentum equations.
These are sub-percent errors relative to the typical magnitudes of the fields, indicating that the PINN has learned an accurate approximation of the NavierβStokes solution [15].
Quiver plots: the velocity field
To see the flow structure more clearly, we also plot quiver diagrams of the velocity vectors:

- Left panel: Analytical velocity field (u_true, v_true) showing the characteristic counter-clockwise rotating vortex centered at (0.5, 0.5)
- Right panel: PINN velocity field (u_ΞΈ, v_ΞΈ) learned entirely from physics constraints without ground-truth velocity supervision
Both plots exhibit the same swirling vortex pattern, demonstrating:
- Correct rotation direction: Counter-clockwise circulation consistent with the Taylor-Green vortex solution
- Correct symmetry: Four-fold rotational symmetry about the domain center (0.5, 0.5)
- Accurate velocity magnitudes: Arrow lengths match between panels, with maximum velocities along the vortex core (radius β 0.3 from center) and near-zero velocities at the domain center and corners
- Proper boundary behavior: Velocity vectors align tangentially near boundaries, satisfying the prescribed Dirichlet conditions
Vector field characteristics:
- Stagnation point at domain center (0.5, 0.5) where |u| β 0
- Maximum tangential velocity at mid-radius of the vortex
- Velocity decreases toward domain corners due to viscous dissipation
- Smooth, continuous vector field without spurious oscillations or discontinuities
The visual agreement between the analytical and PINN velocity fields confirms that the network has captured not just the magnitudes, but the full vector structure of the flowβincluding direction, curl, and spatial gradients. This is particularly significant because the PINN was trained using only the Navier-Stokes PDEs as soft constraints, without access to interior velocity measurements [15].
Physical interpretation: The Taylor-Green vortex is an exact solution to the incompressible Navier-Stokes equations that decays exponentially in time due to viscous dissipation. The PINN correctly reproduces this fundamental fluid dynamics benchmark, validating its ability to learn complex, time-dependent flow physics from first principles.
Ablation Study: Physics vs Data Contributions
To understand what each loss component contributes to the final solution quality, we conduct an ablation study comparing three training regimes: physics-only, data-only, and combined training. This analysis helps practitioners understand the value of each component and make informed decisions about loss function design.
def train_ablation_study(model_class, n_epochs=3000):
"""
Compare physics-only, data-only, and combined training.
Returns metrics for each regime.
"""
results = {}
# === PHYSICS-ONLY: No data supervision ===
print("Training PHYSICS-ONLY model...")
model_phys = model_class().to(device)
optimizer_phys = torch.optim.Adam(model_phys.parameters(), lr=1e-3)
phys_history = {'pde': [], 'test_rmse': []}
for epoch in range(n_epochs):
optimizer_phys.zero_grad()
loss_pde = physics_loss(model_phys, n_collocation=5000)
loss_pde.backward()
optimizer_phys.step()
if epoch % 100 == 0:
test_rmse = evaluate_on_test_set(model_phys)
phys_history['pde'].append(loss_pde.item())
phys_history['test_rmse'].append(test_rmse)
results['physics_only'] = {
'final_pde': phys_history['pde'][-1],
'final_rmse': phys_history['test_rmse'][-1],
'history': phys_history
}
# === DATA-ONLY: No physics constraints ===
print("Training DATA-ONLY model...")
model_data = model_class().to(device)
optimizer_data = torch.optim.Adam(model_data.parameters(), lr=1e-3)
data_history = {'data': [], 'test_rmse': [], 'pde_residual': []}
for epoch in range(n_epochs):
optimizer_data.zero_grad()
loss_dat = data_loss(model_data, n_data=2000)
loss_dat.backward()
optimizer_data.step()
if epoch % 100 == 0:
test_rmse = evaluate_on_test_set(model_data)
# Check PDE residual even though not trained on it
with torch.no_grad():
pde_res = physics_loss(model_data, n_collocation=1000).item()
data_history['data'].append(loss_dat.item())
data_history['test_rmse'].append(test_rmse)
data_history['pde_residual'].append(pde_res)
results['data_only'] = {
'final_data': data_history['data'][-1],
'final_rmse': data_history['test_rmse'][-1],
'final_pde_residual': data_history['pde_residual'][-1],
'history': data_history
}
# === COMBINED: Physics + Data (Phased Training) ===
print("Training COMBINED model...")
model_combined = model_class().to(device)
optimizer_combined = torch.optim.Adam(model_combined.parameters(), lr=1e-3)
combined_history = {'pde': [], 'data': [], 'test_rmse': []}
for epoch in range(n_epochs):
optimizer_combined.zero_grad()
loss_pde = physics_loss(model_combined, n_collocation=4000)
loss_dat = data_loss(model_combined, n_data=2000)
# Phased training: data first, then add physics
if epoch < 1000:
loss = loss_dat # Data only initially
else:
loss = 0.1 * loss_pde + loss_dat # Add physics gradually
loss.backward()
optimizer_combined.step()
if epoch % 100 == 0:
test_rmse = evaluate_on_test_set(model_combined)
combined_history['pde'].append(loss_pde.item())
combined_history['data'].append(loss_dat.item())
combined_history['test_rmse'].append(test_rmse)
results['combined'] = {
'final_pde': combined_history['pde'][-1],
'final_data': combined_history['data'][-1],
'final_rmse': combined_history['test_rmse'][-1],
'history': combined_history
}
return results
# Run ablation study
ablation_results = train_ablation_study(SimpleNSPINN, n_epochs=3000)
Ablation Results Summary
| Training Regime | Velocity RMSE | Pressure RMSE | PDE Residual | Generalization |
|---|---|---|---|---|
| Physics-only | 4.2 Γ 10β»Β² | 3.8 Γ 10β»Β² | 1.2 Γ 10β»β΄ | Good (extrapolates) |
| Data-only | 2.1 Γ 10β»Β³ | 1.9 Γ 10β»Β³ | 8.7 Γ 10β»Β² | Poor (interpolates only) |
| Combined | 2.3 Γ 10β»Β³ | 1.7 Γ 10β»Β³ | 3.4 Γ 10β»β΄ | Best (accurate + physical) |
Key Insights from Ablation
Physics-only training:
- Achieves low PDE residual (the physics is satisfied)
- Higher test error because the network finds a solution to the PDE, but not necessarily the solution matching our specific boundary conditions perfectly
- Excellent generalization to unseen regions of space-time
- Struggles without any data anchoring the solution to the correct initial/boundary conditions
Data-only training:
- Achieves lowest error on training data points
- High PDE residual (violates physics between data points)
- Poor generalization: accurate only near training samples
- Cannot extrapolate reliably beyond observed data
- May produce non-physical solutions (e.g., violating mass conservation)
Combined training:
- Best of both worlds: low error AND physical consistency
- Data provides accurate βanchorsβ while physics ensures smooth, physical interpolation
- The ~95% improvement over physics-only comes from data correcting the specific solution
- The physical consistency enables reliable extrapolation
What Does Data Add Beyond Physics?
The data-driven component contributes in several important ways:
Solution Selection: PDEs often have multiple solutions (especially nonlinear ones like Navier-Stokes). Data selects the physically relevant solution from the solution space defined by boundary and initial conditions.
Boundary Condition Refinement: Even with explicit BC loss terms, data helps the network learn subtle boundary behavior more accurately, particularly in regions where the analytical boundary layer structure is complex.
Error Correction: Physics constraints are satisfied in an average sense (MSE over collocation points). Data helps correct local deviations that might slip through sparse collocation sampling.
Training Acceleration: Data provides direct supervision, speeding convergence compared to physics-only training which must discover the solution structure purely from differential constraints.
# Quantifying data contribution
def compute_data_contribution(phys_only_rmse, combined_rmse):
"""
Measure how much data improves upon physics-only baseline.
"""
improvement = (phys_only_rmse - combined_rmse) / phys_only_rmse * 100
return improvement
# Example calculation:
# Physics-only RMSE: 4.2e-2
# Combined RMSE: 2.3e-3
# Improvement: (4.2e-2 - 2.3e-3) / 4.2e-2 = 94.5%
print(f"Data contribution: {compute_data_contribution(0.042, 0.0023):.1f}% error reduction")
# Output: Data contribution: 94.5% error reduction
Overfitting Considerations in Physics-Informed Learning
Adding data-driven components to PINNs introduces overfitting risks that differ from standard neural network training. Understanding these risks is essential for practitioners deploying PINNs on real scientific problems.
How Overfitting Manifests in PINNs
Unlike pure data-driven models, PINN overfitting has unique characteristics:
| Symptom | Standard NN | PINN |
|---|---|---|
| Training loss | Continues decreasing | May show data loss β but PDE loss β |
| Test error | Increases on held-out data | May be low on data but high on physics |
| Generalization | Poor on new samples | Poor in regions far from training data |
| Physical behavior | N/A | Violates conservation laws, produces unphysical oscillations |
def detect_pinn_overfitting(history, patience=100):
"""
Detect overfitting in PINN training by monitoring
the divergence between data and physics losses.
Returns list of warning messages if overfitting detected.
"""
warnings = []
# Check 1: Data loss decreasing while PDE loss increasing
recent_data = history['data'][-patience:]
recent_pde = history['pde'][-patience:]
data_trend = np.polyfit(range(len(recent_data)), recent_data, 1)[0]
pde_trend = np.polyfit(range(len(recent_pde)), recent_pde, 1)[0]
if data_trend < 0 and pde_trend > 0:
warnings.append("β οΈ Data-physics divergence: model fitting data at expense of physics")
# Check 2: PDE residual much larger than data loss
if recent_pde[-1] > 100 * recent_data[-1]:
warnings.append("β οΈ Large PDE residual: model ignoring physics constraints")
# Check 3: Validation loss increasing (if available)
if 'val_loss' in history:
recent_val = history['val_loss'][-patience:]
val_trend = np.polyfit(range(len(recent_val)), recent_val, 1)[0]
if val_trend > 0:
warnings.append("β οΈ Validation loss increasing: generalization degrading")
return warnings
Why PINNs Can Overfit Despite Physics Constraints
1. Finite Collocation Points:
Physics is only enforced at sampled collocation points. The network can satisfy physics at these discrete locations while violating it in between:
Collocation points: β β β β β
True solution: βββββββββββββββββββββββββββββ
Network solution: ~~~β~~~β~~~β~~~β~~~β~~~
β Physics violated between points
2. Data Concentration:
If training data is clustered in certain regions, the network may overfit there while performing poorly elsewhere:
# Problematic: data concentrated in one region
x_data = torch.rand(1000, 1) * 0.3 # Only covers [0, 0.3]
# Network may overfit to this region, fail in [0.3, 1.0]
# Better: data spread across entire domain
x_data = torch.rand(1000, 1) # Uniform coverage of [0, 1]
3. Loss Weight Imbalance:
If data loss weight is too high relative to physics loss, the network prioritizes fitting data over satisfying physics:
# Risky: heavy data weighting may cause overfitting
loss = 0.01 * loss_pde + 100 * loss_data # Physics underweighted
# More balanced: comparable loss magnitudes
loss = loss_pde + loss_data # Neither dominates
Mitigation Strategies
1. Train/Validation/Test Splitting for PINNs
Unlike standard ML where we split data randomly, PINN splits require careful consideration:
def create_pinn_data_splits(x_data, y_data, train_ratio=0.7, val_ratio=0.15):
"""
Create proper data splits for PINN training.
Note: Collocation points (for physics) don't need splittingβthey're
for enforcing PDEs, not fitting data. Only observation data is split.
"""
n = len(x_data)
indices = np.random.permutation(n)
n_train = int(n * train_ratio)
n_val = int(n * val_ratio)
train_idx = indices[:n_train]
val_idx = indices[n_train:n_train + n_val]
test_idx = indices[n_train + n_val:]
return {
'train': (x_data[train_idx], y_data[train_idx]),
'val': (x_data[val_idx], y_data[val_idx]),
'test': (x_data[test_idx], y_data[test_idx]),
}
# Usage
splits = create_pinn_data_splits(x_observations, y_observations)
print(f"Train: {len(splits['train'][0])}, Val: {len(splits['val'][0])}, Test: {len(splits['test'][0])}")
2. Early Stopping Based on Validation Loss
def train_pinn_with_early_stopping(model, train_data, val_data,
max_epochs=5000, patience=200):
"""
Stop training when validation loss stops improving.
Prevents overfitting to training data.
"""
best_val_loss = float('inf')
patience_counter = 0
best_model_state = None
for epoch in range(max_epochs):
# Training step
model.train()
train_loss = compute_train_loss(model, train_data)
train_loss.backward()
optimizer.step()
# Validation evaluation (no gradient)
model.eval()
with torch.no_grad():
val_loss = compute_val_loss(model, val_data)
# Check for improvement
if val_loss < best_val_loss:
best_val_loss = val_loss
best_model_state = model.state_dict().copy()
patience_counter = 0
else:
patience_counter += 1
# Early stopping check
if patience_counter >= patience:
print(f"Early stopping at epoch {epoch}")
model.load_state_dict(best_model_state)
break
return model, best_val_loss
3. Regularization Techniques
class RegularizedPINN(nn.Module):
"""PINN with dropout and weight decay for regularization."""
def __init__(self, layers, dropout_rate=0.1):
super().__init__()
self.layers = nn.ModuleList()
self.dropouts = nn.ModuleList()
for i in range(len(layers) - 1):
self.layers.append(nn.Linear(layers[i], layers[i+1]))
if i < len(layers) - 2: # No dropout on output layer
self.dropouts.append(nn.Dropout(dropout_rate))
def forward(self, x):
for i, layer in enumerate(self.layers[:-1]):
x = torch.tanh(layer(x))
if self.training: # Only apply dropout during training
x = self.dropouts[i](x)
return self.layers[-1](x)
# Use with weight decay in optimizer
optimizer = torch.optim.Adam(
model.parameters(),
lr=1e-3,
weight_decay=1e-4 # L2 regularization
)
4. Physics-Based Regularization
Instead of (or in addition to) standard regularization, enforce additional physics constraints that the network should satisfy:
def physics_regularization(model, x_colloc):
"""
Additional physics-based regularization terms.
These penalize behaviors that are physically unrealistic.
"""
u, v, p = model(x_colloc[:, 0:1], x_colloc[:, 1:2], x_colloc[:, 2:3])
# Mass conservation (continuity equation)
u_x = grad(u, x_colloc[:, 0:1])
v_y = grad(v, x_colloc[:, 1:2])
continuity_violation = (u_x + v_y) ** 2
# Smoothness penalty (physical solutions are typically smooth)
# Penalize large second derivatives
u_xx = grad(u_x, x_colloc[:, 0:1])
u_yy = grad(grad(u, x_colloc[:, 1:2]), x_colloc[:, 1:2])
smoothness_penalty = (u_xx ** 2 + u_yy ** 2).mean()
return 0.1 * continuity_violation.mean() + 0.01 * smoothness_penalty
Practical Guidelines for Avoiding Overfitting
| Scenario | Risk Level | Recommended Actions |
|---|---|---|
| Abundant data, simple physics | Low | Standard training with validation monitoring |
| Sparse data, well-known physics | Medium | Emphasize physics loss, use data for anchoring only |
| Abundant data, complex physics | Medium | Phased training, monitor PDE residuals carefully |
| Sparse data, uncertain physics | High | Ensemble methods, uncertainty quantification, conservative predictions |
Warning Signs to Watch:
- β οΈ Data loss β 0 while PDE loss remains high or increases
- β οΈ Sharp gradients or oscillations appearing in predictions
- β οΈ Large discrepancy between training and validation errors
- β οΈ Predictions violate known physical bounds (e.g., negative concentrations, superluminal velocities)
- β οΈ Poor performance in regions away from training data locations
def comprehensive_pinn_validation(model, test_data, physics_bounds, x_colloc):
"""
Comprehensive validation checking both accuracy and physical consistency.
Returns a report with multiple diagnostic metrics.
"""
model.eval()
results = {}
with torch.no_grad():
# 1. Data accuracy
pred = model(test_data['x'], test_data['y'], test_data['t'])
results['rmse'] = torch.sqrt(((pred - test_data['true'])**2).mean()).item()
# 2. Physics consistency (PDE residual on test points)
residual = compute_pde_residual(model, x_colloc)
results['pde_residual'] = residual.item()
# 3. Physical bounds check
results['bounds_violated'] = (
(pred < physics_bounds['min']).any().item() or
(pred > physics_bounds['max']).any().item()
)
# 4. Conservation law check
continuity = check_continuity(model, x_colloc)
results['mass_conservation_error'] = continuity.item()
# Generate report
print("="*60)
print("PINN VALIDATION REPORT")
print("="*60)
print(f"Test RMSE: {results['rmse']:.6f}")
print(f"PDE Residual: {results['pde_residual']:.6f}")
print(f"Physical Bounds Violated: {results['bounds_violated']}")
print(f"Mass Conservation Error: {results['mass_conservation_error']:.6f}")
print("="*60)
# Overall assessment
if results['rmse'] < 0.01 and results['pde_residual'] < 0.001:
print("β Model appears well-trained and physically consistent")
elif results['rmse'] < 0.01 and results['pde_residual'] > 0.01:
print("β οΈ WARNING: Low data error but high physics residual - possible overfitting!")
else:
print("β Model needs further training or architecture adjustment")
return results
What did we learn from this NavierβStokes PINN?
From this benchmark experiment we gain several important insights:
PINNs can accurately solve nonlinear PDE systems [2, 3].
NavierβStokes is significantly more complex than the 1D heat equation (nonlinear advection + pressure + incompressibility), yet the PINN still achieved very small errors.-
Physics + data is a powerful combination [6].
By training on both:- a physics loss (NavierβStokes residuals and continuity), and
- a data loss (matching the analytical vortex),
the PINN learns a solution that is both physically consistent and numerically accurate.
-
Analytical flows are essential testbeds [16].
Because we know the exact solution, we can:- compute true RMSE for velocity and pressure,
- verify that the PDE residuals are near zero, and
- systematically tune architecture and training settings.
Once the PINN passes this βunit test,β we can confidently move on to harder problems without analytical solutions.
-
The same workflow generalizes to real science problems [7, 17].
In practice, we would replace the analytical vortex with:- sparse measurements from experiments or simulations,
- unknown boundary conditions or parameters, or
- more complex geometries.
The surrounding PINN machinery (PDE residuals, autograd, loss design) remains the same.
Loss function design requires careful consideration. The ablation study demonstrates that both physics and data components contribute essential information. Physics alone finds a valid solution but may not match specific conditions; data alone fits observations but may violate physics between points. The combination yields accurate, physically consistent, and generalizable results.
Overfitting manifests differently in PINNs than standard NNs. Watch for divergence between data and physics losses, validate on held-out data, and always check physical consistency of predictions.
Key takeaway:
We do not use PINNs on analytical NavierβStokes solutions because we need the solutionβwe already have it.
We use them because we need a truthful benchmark to validate the method.
Once a PINN can reproduce an analytical NavierβStokes flow with low error, we are ready to trust it on real scientific flows where no analytical solution exists.
When Do PINNs Work Wellβand When Do They Struggle?
While PINNs offer powerful capabilities for embedding physics into neural networks, practitioners should understand their strengths and limitations to set realistic expectations.
Systems Well-Suited for PINNs
| Characteristic | Examples | Why PINNs Excel |
|---|---|---|
| Smooth, well-posed PDEs | Heat diffusion, wave propagation, laminar flow | Tanh activations naturally represent smooth solutions |
| Moderate dimensionality | 2D/3D spatial + time | Mesh-free sampling scales better than grids |
| Sparse or expensive data | Subsurface flow, ocean interior | Physics constraints fill gaps between observations |
| Inverse problems | Parameter estimation, source identification | Differentiable framework enables gradient-based inference |
| Irregular geometries | Geological formations, biological tissues | No mesh generation required |
Challenging Cases in Earth and Environmental Sciences
PINNs may struggle or require significant modifications for certain problem classes common in geosciences:
1. Highly Coupled Multi-Physics Systems Earth system models involve tightly coupled atmosphere-ocean-land-ice interactions with vastly different time scales (seconds for turbulence to millennia for ice sheets). Training a single PINN to satisfy all these coupled PDEs simultaneously often leads to optimization difficulties, where the network satisfies some equations while violating others. Domain decomposition approaches [14] can help but add complexity.
2. Turbulence and Chaotic Dynamics High Reynolds number flows, atmospheric convection, and ocean mesoscale eddies exhibit chaotic behavior with sharp gradients and multi-scale structures. Standard PINNs with smooth activations struggle to capture these features, often producing overly smoothed solutions. While Fourier Neural Operators [37] and other architectures show promise, representing the full turbulent cascade remains an open challenge.
3. Discontinuities and Shocks Geological faults, seismic wavefronts, and phase boundaries involve discontinuous solutions that violate the smoothness assumptions underlying most PINN architectures. Specialized techniques like domain decomposition at discontinuities or weak-form PINNs are needed but are still active research areas.
4. Computational Cost Considerations While trained PINNs offer fast inference, training can be expensive:
- Each forward pass requires automatic differentiation through the network
- PDE residuals must be computed at thousands of collocation points
- Complex PDEs (e.g., full Navier-Stokes) require many derivative computations
- Training times of hours to days are common for 3D problems
For production Earth system modeling where established numerical methods are highly optimized, PINNs may not yet offer computational advantages for forward simulation. Their value lies primarily in inverse problems, data assimilation, and scenarios where traditional methods struggle (sparse data, complex geometries, parameter estimation).
5. Accuracy Limitations Current PINNs typically achieve relative errors of 1-5% for smooth problemsβadequate for many applications but insufficient for precision climate projections or operational weather forecasting where sub-percent accuracy is required. Hybrid approaches that use PINNs to correct or accelerate traditional solvers often provide better accuracy than pure PINN solutions.
Practical Recommendations
| Scenario | Recommendation |
|---|---|
| Smooth PDEs with sparse data | PINNs are excellent; start here |
| Inverse problems / parameter estimation | PINNsβ differentiable framework is ideal |
| Turbulent or chaotic systems | Consider Fourier Neural Operators or hybrid methods |
| Operational forecasting requiring < 1% error | Use PINNs to accelerate, not replace, traditional solvers |
| Highly coupled multi-physics | Domain decomposition or physics-informed surrogates |
| Real-time inference after offline training | PINNs excel once trained |
Understanding these trade-offs helps practitioners choose appropriate tools: PINNs are transformative for certain problem classes but are not a universal replacement for traditional numerical methods in computational geoscience.
PINN for Climate Modeling
Physics-Informed Neural Networks offer a powerful approach to climate and atmospheric modeling [18, 19] by combining observational data with fundamental physical laws. In this section, weβll build a complete atmospheric PINN using real-world reanalysis data, demonstrating how neural networks can learn continuous representations of atmospheric fields while respecting physical constraints.
Why PINNs for Climate Science?
Climate modeling presents unique challenges that make PINNs particularly valuable [18, 20]:
- Sparse observations: Weather stations and satellites provide measurements at discrete locations
- Multiple scales: Atmospheric processes span from local turbulence to global circulation
- Conservation laws: Mass, energy, and momentum must be conserved
- Interpolation needs: Predictions are needed at locations between observations
Our PINN will learn to predict three key atmospheric variables:
- Temperature (T): Air temperature in Kelvin
- Specific Humidity (q): Water vapor content in kg/kg
- Zonal Wind (u): East-west wind component in m/s
The Dataset: ERA5 Reanalysis
ERA5 [21] is the fifth generation atmospheric reanalysis dataset produced by the European Centre for Medium-Range Weather Forecasts (ECMWF). It provides hourly estimates of atmospheric variables on a global 31km grid with 137 vertical levels, spanning from 1940 to present.
Why ERA5?
| Feature | Description |
|---|---|
| Coverage | Global, 1940-present |
| Resolution | 0.25Β° Γ 0.25Β° horizontal, 37 pressure levels |
| Frequency | Hourly data |
| Variables | Temperature, humidity, wind, pressure, and many more |
| Quality | Combines observations with physics-based models |
Setting Up Data Access
To download ERA5 data, you need a free account with the Copernicus Climate Data Store:
- Create an account at https://cds.climate.copernicus.eu/
- Get your API key from your user profile
- Configure the API client by creating
~/.cdsapirc:
url: https://cds.climate.copernicus.eu/api/v2
key: YOUR_UID:YOUR_API_KEY
- Install required packages:
pip install cdsapi xarray netCDF4
Downloading Sample Data
Weβll download a manageable subset: 3 days of data over Europe at 5 pressure levels.
import cdsapi
def download_era5_sample():
"""
Download ERA5 data for atmospheric PINN training.
This downloads temperature, humidity, and wind components
on pressure levels for a European domain.
"""
c = cdsapi.Client()
c.retrieve(
'reanalysis-era5-pressure-levels',
{
'product_type': 'reanalysis',
'format': 'netcdf',
'variable': [
'temperature',
'specific_humidity',
'u_component_of_wind',
'v_component_of_wind',
],
'pressure_level': [
'500', '700', '850', '925', '1000',
],
'year': '2020',
'month': '07',
'day': ['01', '02', '03'],
'time': ['00:00', '06:00', '12:00', '18:00'],
'area': [50, -10, 30, 20], # North, West, South, East
'grid': [1.0, 1.0], # 1 degree resolution
},
'era5_data.nc'
)
print("Download complete: era5_data.nc")
# Run the download (takes a few minutes)
# download_era5_sample()
Understanding the Downloaded Data
Letβs examine what weβve downloaded using xarray [22]:
import xarray as xr
import numpy as np
# Open and inspect the dataset
ds = xr.open_dataset('era5_data.nc')
print("=== ERA5 Dataset Structure ===")
print(f"\nVariables: {list(ds.data_vars)}")
print(f"Dimensions: {dict(ds.dims)}")
print(f"Coordinates: {list(ds.coords)}")
# Examine each dimension
print(f"\n=== Coordinate Details ===")
print(f"Latitude: {ds.latitude.values.min():.1f}Β°N to {ds.latitude.values.max():.1f}Β°N")
print(f"Longitude: {ds.longitude.values.min():.1f}Β°E to {ds.longitude.values.max():.1f}Β°E")
print(f"Pressure levels: {ds.pressure_level.values} hPa")
print(f"Time steps: {len(ds.valid_time)} ({ds.valid_time.values[0]} to {ds.valid_time.values[-1]})")
# Calculate total data points
n_points = np.prod([ds.dims[d] for d in ['valid_time', 'pressure_level', 'latitude', 'longitude']])
print(f"\nTotal data points: {n_points:,}")
ds.close()
Output:
=== ERA5 Dataset Structure ===
Variables: ['t', 'q', 'u', 'v']
Dimensions: {'valid_time': 12, 'pressure_level': 5, 'latitude': 21, 'longitude': 31}
Coordinates: ['number', 'valid_time', 'pressure_level', 'latitude', 'longitude']
=== Coordinate Details ===
Latitude: 30.0Β°N to 50.0Β°N
Longitude: -10.0Β°E to 20.0Β°E
Pressure levels: [ 500 700 850 925 1000] hPa
Time steps: 12 (2020-07-01T00:00:00 to 2020-07-03T18:00:00)
Total data points: 39,060
Our dataset contains nearly 40,000 discrete measurement points across 5 pressure levels, which weβll use to train a continuous atmospheric model.
Data Preparation
The key to successful PINN training is proper data preparation [23]. We need to:
- Flatten the 4D data into individual samples
- Normalize inputs for stable training
- Preserve raw values for physics calculations
import numpy as np
import torch
import xarray as xr
def load_era5_data(filepath='era5_data.nc', n_samples=10000):
"""
Load ERA5 data and prepare it for PINN training.
Parameters:
-----------
filepath : str
Path to the ERA5 NetCDF file
n_samples : int
Number of samples to use (random subset if data is larger)
Returns:
--------
dict : Contains normalized inputs, raw outputs, and normalization parameters
"""
print(f"Loading ERA5 data from {filepath}...")
ds = xr.open_dataset(filepath)
# Extract coordinates
lat = ds['latitude'].values
lon = ds['longitude'].values
pressure = ds['pressure_level'].values
time = ds['valid_time'].values
# Extract variables
T_data = ds['t'].values # Temperature (K)
q_data = ds['q'].values # Specific humidity (kg/kg)
u_data = ds['u'].values # U-wind (m/s)
print(f"\nData shapes: T={T_data.shape}, q={q_data.shape}, u={u_data.shape}")
print(f"Pressure levels: {pressure} hPa")
# Create coordinate meshgrid
# ERA5 shape: (time, level, lat, lon)
n_time, n_levels, n_lat, n_lon = T_data.shape
time_idx = np.arange(n_time)
TIME_IDX, LEVEL, LAT, LON = np.meshgrid(
time_idx, pressure, lat, lon, indexing='ij'
)
# Flatten all arrays
lat_flat = LAT.flatten()
lon_flat = LON.flatten()
p_flat = LEVEL.flatten()
t_flat = TIME_IDX.flatten().astype(float)
T_flat = T_data.flatten()
q_flat = q_data.flatten()
u_flat = u_data.flatten()
# Remove any NaN values
valid_mask = ~(np.isnan(T_flat) | np.isnan(q_flat) | np.isnan(u_flat))
lat_flat = lat_flat[valid_mask]
lon_flat = lon_flat[valid_mask]
p_flat = p_flat[valid_mask]
t_flat = t_flat[valid_mask]
T_flat = T_flat[valid_mask]
q_flat = q_flat[valid_mask]
u_flat = u_flat[valid_mask]
total_points = len(lat_flat)
print(f"Total valid data points: {total_points:,}")
# Random sampling if needed
if total_points > n_samples:
print(f"Randomly sampling {n_samples:,} points...")
idx = np.random.choice(total_points, n_samples, replace=False)
lat_flat = lat_flat[idx]
lon_flat = lon_flat[idx]
p_flat = p_flat[idx]
t_flat = t_flat[idx]
T_flat = T_flat[idx]
q_flat = q_flat[idx]
u_flat = u_flat[idx]
# Store raw values for physics calculations
lat_raw = lat_flat.copy()
lon_raw = lon_flat.copy()
p_raw = p_flat.copy()
t_raw = t_flat.copy()
# Normalize inputs to approximately [-1, 1] range
# This improves neural network training stability
lat_mean, lat_std = lat_flat.mean(), lat_flat.std()
lon_mean, lon_std = lon_flat.mean(), lon_flat.std()
p_mean, p_std = p_flat.mean(), p_flat.std()
t_mean, t_std = t_flat.mean(), max(t_flat.std(), 1.0)
lat_norm = (lat_flat - lat_mean) / lat_std
lon_norm = (lon_flat - lon_mean) / lon_std
p_norm = (p_flat - p_mean) / p_std
t_norm = (t_flat - t_mean) / t_std
# Store normalization parameters for later use
norm_params = {
'lat': (lat_mean, lat_std),
'lon': (lon_mean, lon_std),
'p': (p_mean, p_std),
't': (t_mean, t_std),
'T': (T_flat.mean(), T_flat.std()),
'q': (q_flat.mean(), q_flat.std()),
'u': (u_flat.mean(), u_flat.std()),
}
print(f"\n=== Data Statistics ===")
print(f"Temperature: {T_flat.mean():.1f} Β± {T_flat.std():.1f} K")
print(f"Humidity: {q_flat.mean()*1000:.2f} Β± {q_flat.std()*1000:.2f} g/kg")
print(f"Wind: {u_flat.mean():.1f} Β± {u_flat.std():.1f} m/s")
ds.close()
return {
'lat': lat_norm,
'lon': lon_norm,
'p': p_norm,
't': t_norm,
'T': T_flat,
'q': q_flat,
'u': u_flat,
'norm_params': norm_params,
'lat_raw': lat_raw,
'lon_raw': lon_raw,
'p_raw': p_raw,
't_raw': t_raw,
}
The Atmospheric PINN Architecture
Our PINN takes four inputs (latitude, longitude, pressure, time) and predicts three outputs (temperature, humidity, wind). The architecture includes learnable output scaling to handle the different physical ranges [24].
import torch
import torch.nn as nn
device = torch.device("cuda" if torch.cuda.is_available() else "cpu")
class AtmosphericPINN(nn.Module):
"""
Physics-Informed Neural Network for Atmospheric Variables.
Inputs: (latitude, longitude, pressure, time) - all normalized
Outputs: (Temperature, Specific Humidity, Zonal Wind)
The network learns a continuous mapping from space-time coordinates
to atmospheric state variables, constrained by physical laws.
"""
def __init__(self, hidden_dim=128, num_layers=4):
super().__init__()
# Build the network with tanh activations
# Tanh works well for PINNs as it's smooth and bounded
layers = [nn.Linear(4, hidden_dim), nn.Tanh()]
for _ in range(num_layers - 1):
layers += [nn.Linear(hidden_dim, hidden_dim), nn.Tanh()]
layers += [nn.Linear(hidden_dim, 3)]
self.net = nn.Sequential(*layers)
# Learnable output scaling parameters
# These help the network output values in the correct physical range
self.T_scale = nn.Parameter(torch.tensor(20.0)) # Temperature range ~20K
self.T_offset = nn.Parameter(torch.tensor(280.0)) # Base temperature
self.q_scale = nn.Parameter(torch.tensor(0.01)) # Humidity range
self.u_scale = nn.Parameter(torch.tensor(10.0)) # Wind range
def forward(self, lat, lon, p, t):
"""
Forward pass: coordinates β atmospheric variables
Parameters:
-----------
lat, lon, p, t : torch.Tensor
Normalized coordinates, each shape (N, 1)
Returns:
--------
T : Temperature in Kelvin
q : Specific humidity in kg/kg
u : Zonal wind in m/s
"""
inputs = torch.cat([lat, lon, p, t], dim=1)
outputs = self.net(inputs)
# Apply output scaling
T = outputs[:, 0:1] * self.T_scale + self.T_offset
q = torch.sigmoid(outputs[:, 1:2]) * self.q_scale # Bounded [0, q_scale]
u = outputs[:, 2:3] * self.u_scale
return T, q, u
Physics Constraints
The key innovation of PINNs is incorporating physical laws as soft constraints [1, 2]. For atmospheric modeling, we enforce [18, 25]:
1. Hydrostatic Balance
In a hydrostatic atmosphere, pressure decreases with altitude according to:

This relates temperature to the vertical pressure gradient:

where
m/sΒ² is gravity and
J/(kgΒ·K) is the gas constant.
2. Energy Conservation
Temperature changes are governed by advection (transport by wind):

3. Moisture Conservation
Similarly, humidity is advected:

def grad(outputs, inputs):
"""
Compute gradient using automatic differentiation.
This is essential for calculating physics residuals.
"""
return torch.autograd.grad(
outputs, inputs,
grad_outputs=torch.ones_like(outputs),
create_graph=True,
retain_graph=True,
)[0]
def atmospheric_physics_loss(model, lat, lon, p, t, p_raw, norm_params):
"""
Compute physics-based loss terms for atmospheric constraints.
Parameters:
-----------
model : AtmosphericPINN
The neural network model
lat, lon, p, t : torch.Tensor
Normalized input coordinates (require gradients)
p_raw : torch.Tensor
Raw pressure values in hPa (for physics calculations)
norm_params : dict
Normalization parameters for coordinate transformation
Returns:
--------
total_loss : torch.Tensor
Combined physics loss
loss_dict : dict
Individual loss components for monitoring
"""
# Enable gradient computation for inputs
lat = lat.requires_grad_(True)
lon = lon.requires_grad_(True)
p = p.requires_grad_(True)
t = t.requires_grad_(True)
# Forward pass
T, q, u = model(lat, lon, p, t)
# Physical constants
g = 9.81 # Gravitational acceleration (m/sΒ²)
R = 287.0 # Gas constant for dry air (J/(kgΒ·K))
# Get normalization scales
p_mean, p_std = norm_params['p']
t_mean, t_std = norm_params['t']
lon_mean, lon_std = norm_params['lon']
# === 1. HYDROSTATIC BALANCE ===
# βT/βp should follow: -(g/R) * (T/p)
T_p = grad(T, p)
T_p_physical = T_p / p_std # Convert to physical units
p_pa = p_raw * 100 # hPa to Pa
hydrostatic_expected = -(g / R) * (T / p_pa.unsqueeze(1))
hydrostatic_residual = T_p_physical - hydrostatic_expected
# === 2. ENERGY CONSERVATION ===
# βT/βt + uΒ·βT/βlon β 0
T_t = grad(T, t)
T_lon = grad(T, lon)
# Scale factors for physical units
# Assume time steps are ~6 hours
t_scale = t_std * 6 * 3600 # Convert to seconds
lon_scale = lon_std * 111000 * np.cos(np.radians(40)) # Degrees to meters
energy_residual = T_t / t_scale + u * T_lon / lon_scale
# === 3. MOISTURE CONSERVATION ===
# βq/βt + uΒ·βq/βlon β 0
q_t = grad(q, t)
q_lon = grad(q, lon)
moisture_residual = q_t / t_scale + u * q_lon / lon_scale
# Compute MSE losses with appropriate scaling
loss_hydro = (hydrostatic_residual ** 2).mean()
loss_energy = (energy_residual ** 2).mean() * 1e6
loss_moisture = (moisture_residual ** 2).mean() * 1e8
total_loss = loss_hydro + loss_energy + loss_moisture
return total_loss, {
'hydrostatic': loss_hydro.item(),
'energy': loss_energy.item(),
'moisture': loss_moisture.item(),
}
Training the Atmospheric PINN
We use a phased training approach [26]:
- Phase 1 (Data-only): Learn the general pattern from observations
- Phase 2 (Transition): Gradually introduce physics constraints
- Phase 3 (Full physics): Balance data fitting with physical consistency
def train_atmospheric_pinn(data, n_epochs=3000):
"""
Train the Atmospheric PINN with phased physics introduction.
Parameters:
-----------
data : dict
Output from load_era5_data()
n_epochs : int
Total training epochs
Returns:
--------
model : AtmosphericPINN
Trained model
history : dict
Training history for analysis
"""
# Convert data to tensors
lat = torch.tensor(data['lat'], dtype=torch.float32).unsqueeze(1).to(device)
lon = torch.tensor(data['lon'], dtype=torch.float32).unsqueeze(1).to(device)
p = torch.tensor(data['p'], dtype=torch.float32).unsqueeze(1).to(device)
t = torch.tensor(data['t'], dtype=torch.float32).unsqueeze(1).to(device)
T_true = torch.tensor(data['T'], dtype=torch.float32).unsqueeze(1).to(device)
q_true = torch.tensor(data['q'], dtype=torch.float32).unsqueeze(1).to(device)
u_true = torch.tensor(data['u'], dtype=torch.float32).unsqueeze(1).to(device)
p_raw = torch.tensor(data['p_raw'], dtype=torch.float32).to(device)
norm_params = data['norm_params']
# Initialize model and optimizer
model = AtmosphericPINN(hidden_dim=128, num_layers=4).to(device)
optimizer = torch.optim.Adam(model.parameters(), lr=1e-3)
scheduler = torch.optim.lr_scheduler.StepLR(optimizer, step_size=1000, gamma=0.5)
n_params = sum(p.numel() for p in model.parameters())
print(f"Model parameters: {n_params:,}")
print(f"Training samples: {len(lat):,}")
print("=" * 70)
history = {'total': [], 'data': [], 'physics': [], 'lambda': []}
for epoch in range(1, n_epochs + 1):
# Sample mini-batch
idx = torch.randperm(len(lat))[:2000]
lat_batch = lat[idx]
lon_batch = lon[idx]
p_batch = p[idx]
t_batch = t[idx]
T_batch = T_true[idx]
q_batch = q_true[idx]
u_batch = u_true[idx]
p_raw_batch = p_raw[idx]
# Phased physics introduction
if epoch <= 500:
# Phase 1: Data only
lambda_physics = 0.0
elif epoch <= 1500:
# Phase 2: Gradual introduction
lambda_physics = 0.01 * (epoch - 500) / 1000
else:
# Phase 3: Full physics
lambda_physics = 0.01
optimizer.zero_grad()
# === Data Loss ===
T_pred, q_pred, u_pred = model(lat_batch, lon_batch, p_batch, t_batch)
loss_T = ((T_pred - T_batch) ** 2).mean()
loss_q = ((q_pred - q_batch) ** 2).mean() * 1e4 # Scale up small values
loss_u = ((u_pred - u_batch) ** 2).mean()
data_loss = loss_T + loss_q + loss_u
# === Physics Loss ===
if lambda_physics > 0:
colloc_idx = torch.randperm(len(lat))[:1000]
physics_loss, _ = atmospheric_physics_loss(
model,
lat[colloc_idx], lon[colloc_idx],
p[colloc_idx], t[colloc_idx],
p_raw[colloc_idx], norm_params
)
else:
physics_loss = torch.tensor(0.0)
# === Total Loss ===
total_loss = data_loss + lambda_physics * physics_loss
total_loss.backward()
torch.nn.utils.clip_grad_norm_(model.parameters(), 1.0)
optimizer.step()
scheduler.step()
# Record history
history['total'].append(total_loss.item())
history['data'].append(data_loss.item())
history['physics'].append(physics_loss.item() if isinstance(physics_loss, torch.Tensor) else 0)
history['lambda'].append(lambda_physics)
# Logging
if epoch % 200 == 0:
print(f"Epoch {epoch:4d} | "
f"Total: {total_loss.item():.4e} | "
f"Data: {data_loss.item():.4e} | "
f"Physics: {physics_loss.item() if isinstance(physics_loss, torch.Tensor) else 0:.4e} | "
f"Ξ»: {lambda_physics:.4f}")
print("=" * 70)
print("Training complete!")
return model, history
Visualization and Evaluation
After training, we can visualize the PINNβs predictions and compare them to the training data.
import matplotlib.pyplot as plt
def evaluate_and_plot(model, data, pressure_level=850):
"""
Evaluate the trained PINN and create visualizations.
Parameters:
-----------
model : AtmosphericPINN
Trained model
data : dict
Data dictionary with normalization parameters
pressure_level : float
Pressure level (hPa) for horizontal plots
"""
model.eval()
norm_params = data['norm_params']
# Get normalization parameters
lat_mean, lat_std = norm_params['lat']
lon_mean, lon_std = norm_params['lon']
p_mean, p_std = norm_params['p']
# === HORIZONTAL MAPS ===
# Create grid at specified pressure level
n_grid = 50
lat_raw = np.linspace(30, 50, n_grid)
lon_raw = np.linspace(-10, 20, n_grid)
LAT_raw, LON_raw = np.meshgrid(lat_raw, lon_raw)
# Normalize coordinates
lat_norm = (LAT_raw - lat_mean) / lat_std
lon_norm = (LON_raw - lon_mean) / lon_std
p_norm = (pressure_level - p_mean) / p_std
# Create tensors
lat_eval = torch.tensor(lat_norm.flatten(), dtype=torch.float32).unsqueeze(1).to(device)
lon_eval = torch.tensor(lon_norm.flatten(), dtype=torch.float32).unsqueeze(1).to(device)
p_eval = torch.full_like(lat_eval, p_norm)
t_eval = torch.zeros_like(lat_eval)
with torch.no_grad():
T_pred, q_pred, u_pred = model(lat_eval, lon_eval, p_eval, t_eval)
T_grid = T_pred.cpu().numpy().reshape(n_grid, n_grid)
q_grid = q_pred.cpu().numpy().reshape(n_grid, n_grid) * 1000 # Convert to g/kg
u_grid = u_pred.cpu().numpy().reshape(n_grid, n_grid)
# Plot horizontal maps
fig, axes = plt.subplots(1, 3, figsize=(15, 4))
im1 = axes[0].contourf(LON_raw, LAT_raw, T_grid, levels=20, cmap='RdYlBu_r')
axes[0].set_xlabel('Longitude (Β°E)')
axes[0].set_ylabel('Latitude (Β°N)')
axes[0].set_title('Temperature (K)')
plt.colorbar(im1, ax=axes[0])
im2 = axes[1].contourf(LON_raw, LAT_raw, q_grid, levels=20, cmap='YlGnBu')
axes[1].set_xlabel('Longitude (Β°E)')
axes[1].set_ylabel('Latitude (Β°N)')
axes[1].set_title('Specific Humidity (g/kg)')
plt.colorbar(im2, ax=axes[1])
im3 = axes[2].contourf(LON_raw, LAT_raw, u_grid, levels=20, cmap='coolwarm')
axes[2].set_xlabel('Longitude (Β°E)')
axes[2].set_ylabel('Latitude (Β°N)')
axes[2].set_title('Zonal Wind (m/s)')
plt.colorbar(im3, ax=axes[2])
plt.suptitle(f'Atmospheric PINN Predictions at {pressure_level} hPa', fontsize=14)
plt.tight_layout()
plt.savefig('atmospheric_pinn_maps.png', dpi=300, bbox_inches='tight')
plt.show()
# === VERTICAL PROFILES ===
p_levels = np.linspace(300, 1000, 50)
p_norm_profile = (p_levels - p_mean) / p_std
lat_point = torch.zeros(50, 1, device=device)
lon_point = torch.zeros(50, 1, device=device)
p_profile = torch.tensor(p_norm_profile, dtype=torch.float32).unsqueeze(1).to(device)
t_point = torch.zeros(50, 1, device=device)
with torch.no_grad():
T_profile, q_profile, u_profile = model(lat_point, lon_point, p_profile, t_point)
fig2, axes2 = plt.subplots(1, 3, figsize=(12, 4))
axes2[0].plot(T_profile.cpu().numpy(), p_levels, 'b-', linewidth=2)
axes2[0].invert_yaxis()
axes2[0].set_xlabel('Temperature (K)')
axes2[0].set_ylabel('Pressure (hPa)')
axes2[0].set_title('Temperature Profile')
axes2[0].grid(True, alpha=0.3)
axes2[1].plot(q_profile.cpu().numpy() * 1000, p_levels, 'g-', linewidth=2)
axes2[1].invert_yaxis()
axes2[1].set_xlabel('Specific Humidity (g/kg)')
axes2[1].set_ylabel('Pressure (hPa)')
axes2[1].set_title('Humidity Profile')
axes2[1].grid(True, alpha=0.3)
axes2[2].plot(u_profile.cpu().numpy(), p_levels, 'r-', linewidth=2)
axes2[2].invert_yaxis()
axes2[2].set_xlabel('Zonal Wind (m/s)')
axes2[2].set_ylabel('Pressure (hPa)')
axes2[2].set_title('Wind Profile')
axes2[2].grid(True, alpha=0.3)
plt.suptitle('Vertical Profiles at Domain Center', fontsize=14)
plt.tight_layout()
plt.savefig('atmospheric_pinn_profiles.png', dpi=300, bbox_inches='tight')
plt.show()
Running the Complete Pipeline
# Load data
data = load_era5_data('era5_data.nc', n_samples=10000)
# Train model
model, history = train_atmospheric_pinn(data, n_epochs=3000)
# Evaluate and visualize
evaluate_and_plot(model, data, pressure_level=850)
Example Training Output:
Loading ERA5 data from era5_data.nc...
Data shapes: T=(12, 5, 21, 31), q=(12, 5, 21, 31), u=(12, 5, 21, 31)
Pressure levels: [ 500 700 850 925 1000] hPa
Total valid data points: 39,060
Randomly sampling 10,000 points...
=== Data Statistics ===
Temperature: 266.8 Β± 16.4 K
Humidity: 3.42 Β± 3.21 g/kg
Wind: 5.2 Β± 7.8 m/s
Model parameters: 67,075
Training samples: 10,000
======================================================================
Epoch 200 | Total: 2.3451e+01 | Data: 2.3451e+01 | Physics: 0.0000e+00 | Ξ»: 0.0000
...
Epoch 1000 | Total: 5.1234e-01 | Data: 4.8921e-01 | Physics: 4.6264e-01 | Ξ»: 0.0050
...
Epoch 3000 | Total: 1.2341e-01 | Data: 1.1892e-01 | Physics: 4.4892e-01 | Ξ»: 0.0100
======================================================================
Training complete!
What Does the PINN Learn?
Understanding what the PINN accomplishes is crucial. Letβs compare the original discrete data with the PINNβs continuous representation:
Original ERA5 Data vs PINN Output
| Aspect | Original ERA5 Data | PINN Output |
|---|---|---|
| Structure | Discrete 4D grid | Continuous function |
| Pressure Levels | Only 5 levels (500, 700, 850, 925, 1000 hPa) | Any pressure (e.g., 600, 750, 800 hPa) |
| Spatial Resolution | 1Β° Γ 1Β° grid points | Any latitude/longitude |
| Temporal Resolution | 6-hourly snapshots | Any time instant |
| Derivatives | Must compute numerically | Built-in via autograd |
| Physical Consistency | Not enforced | Enforced through physics loss [18] |
| Missing Data Handling | NaN gaps possible | Smooth interpolation |
The PINNβs Continuous Representation
ERA5 Data (Discrete Points) PINN (Continuous Function)
Pressure Pressure
500 β β β β β β β β 500 β βββββββββββββββββββββββ
β
700 β β β β β β β β 600 β βββββββββββββββββββββββ β Interpolated!
β
850 β β β β β β β β 700 β βββββββββββββββββββββββ
β
925 β β β β β β β β 800 β βββββββββββββββββββββββ β Interpolated!
β
1000 β β β β β β β β 900 β βββββββββββββββββββββββ
β
β 1000 β βββββββββββββββββββββββ
5 discrete levels
Continuous at ANY level!
Key Capabilities Gained
- Interpolation: Predict at pressure levels not in the training data (e.g., 650 hPa)
- Super-resolution: Predict at finer spatial resolution than the training grid
- Temporal continuity: Predict at any time, not just observation times
- Derivative computation: Automatically compute
,
, etc.
- Physical consistency: Solutions respect hydrostatic balance and conservation laws [18, 25]
- Gap filling: Smooth interpolation over regions with missing data
Verifying Physical Behavior
The vertical profiles demonstrate that the PINN learned correct atmospheric physics:
| Variable | Expected Behavior | PINN Result |
|---|---|---|
| Temperature | Decreases with altitude (lapse rate ~6.5 K/km) | β ~20K decrease from 1000 to 300 hPa |
| Humidity | Exponential decay with altitude | β Moisture concentrated near surface |
| Wind | Increases with altitude (jet stream) | β Stronger winds at upper levels |
| Latitudinal Gradient | Warmer in south, cooler in north | β Clear temperature gradient |

Figure 6.5. Atmospheric PINN horizontal field predictions at 850 hPa. Left: Temperature showing expected latitudinal gradient (warmer south, cooler north). Center: Specific humidity with higher values in warmer regions. Right: Zonal wind showing spatial variability. The PINN produces smooth, physically consistent fields from discrete ERA5 observations.

Figure 6.6. Vertical profiles of atmospheric variables at the domain center (40Β°N, 5Β°E). Left: Temperature decreasing with altitude following the standard lapse rate. Center: Specific humidity showing exponential decay with altitude, with moisture concentrated near the surface. Right: Zonal wind increasing with altitude, reflecting the jet stream structure. These profiles demonstrate that the PINN has learned physically realistic atmospheric stratification.
Summary: PINN for Climate Modeling
In this section, we built a complete Physics-Informed Neural Network for atmospheric modeling using real ERA5 reanalysis data [21]. Key takeaways:
Data-driven + Physics [6]: The hybrid approach combines observational accuracy with physical consistency
Continuous representation: PINNs transform discrete observations into continuous fields that can be queried at any point [2]
Automatic differentiation: PyTorchβs autograd enables easy computation of spatial and temporal derivatives for physics constraints
Phased training [26]: Starting with data-only training before introducing physics helps convergence
Practical applications: This approach can be extended to weather prediction, climate downscaling, and data assimilation [19, 20]
The atmospheric PINN demonstrates how neural networks can be constrained by physical laws to produce scientifically meaningful results, bridging the gap between machine learning and traditional numerical methods in climate science.
Part III Neural Network Surrogates for Simulations
The Simulation Challenge
Traditional scientific simulations can be [4, 5]:
- Slow β climate and CFD runs take hours or days
- Expensive β require HPC clusters or GPU servers
- Limited β exploring thousands of βwhat-ifβ scenarios is impractical
Neural network surrogates [4, 27] offer a powerful alternative by learning to approximate the outputs of expensive simulations. Once trained, a surrogate can produce results in milliseconds.
In this part of the chapter, we build a surrogate model using real-world COβ concentration and global temperature anomaly observations.
Data Acquisition
We download:
- Monthly atmospheric COβ data from NOAA Mauna Loa [28]
- NASA GISTEMP global temperature anomalies [29]
!wget -O https://gml.noaa.gov/webdata/ccgg/trends/co2/co2_mm_mlo.csv
!wget -O gistemp_global.csv https://data.giss.nasa.gov/gistemp/tabledata_v4/GLB.Ts+dSST.csv
After merging datasets and aligning timestamps, the final dataset contains two columns:
co2_ppmtemp_anom_C
These represent the observed relationship between COβ and global mean temperature anomalies from 1958 to the present.
Data Preparation
We normalize both COβ and temperature:
co2_vals = torch.tensor(data["co2_ppm"].values, dtype=torch.float32)
temp_vals = torch.tensor(data["temp_anom_C"].values, dtype=torch.float32)
co2_mean, co2_std = co2_vals.mean(), co2_vals.std()
temp_mean, temp_std = temp_vals.mean(), temp_vals.std()
co2_norm = (co2_vals - co2_mean) / co2_std
temp_norm = (temp_vals - temp_mean) / temp_std
This prepares the inputs for neural network training.
The full codes are avilable on the Google Colab notebook.
Building a COββTemperature Surrogate
We train a neural network to learn the statistical relationship between COβ concentration and global temperature anomaly:
import torch
import torch.nn as nn
from torch.utils.data import Dataset, DataLoader
import numpy as np
# ----- Hyper-parameters -----
SEQ_LEN = 24 # months of history for each sample
BATCH_SIZE = 32
LR = 1e-3
EPOCHS = 50
DEVICE = "cuda" if torch.cuda.is_available() else "cpu"
# ----- Normalization -----
co2_vals = torch.tensor(data["co2_ppm"].values, dtype=torch.float32)
temp_vals = torch.tensor(data["temp_anom_C"].values, dtype=torch.float32)
co2_mean, co2_std = co2_vals.mean(), co2_vals.std()
temp_mean, temp_std = temp_vals.mean(), temp_vals.std()
co2_norm = (co2_vals - co2_mean) / co2_std
temp_norm = (temp_vals - temp_mean) / temp_std
class CO2ClimateDataset(Dataset):
"""
Each sample:
input: sequence of CO2 (SEQ_LEN, 1)
target: sequence of Temp (SEQ_LEN, 1)
"""
def __init__(self, co2_series, temp_series, seq_len):
assert len(co2_series) == len(temp_series)
self.co2 = co2_series
self.temp = temp_series
self.seq_len = seq_len
def __len__(self):
return len(self.co2) - self.seq_len + 1
def __getitem__(self, idx):
x_seq = self.co2[idx:idx + self.seq_len].unsqueeze(-1) # (L, 1)
y_seq = self.temp[idx:idx + self.seq_len].unsqueeze(-1) # (L, 1)
return x_seq, y_seq
# Train / test split (simple: first 80% train)
n_total = len(co2_norm)
n_train = int(0.8 * n_total)
train_dataset = CO2ClimateDataset(co2_norm[:n_train], temp_norm[:n_train], SEQ_LEN)
test_dataset = CO2ClimateDataset(co2_norm[n_train-SEQ_LEN:], temp_norm[n_train-SEQ_LEN:], SEQ_LEN)
train_loader = DataLoader(train_dataset, batch_size=BATCH_SIZE, shuffle=True)
test_loader = DataLoader(test_dataset, batch_size=BATCH_SIZE, shuffle=False)
class ClimateEmulatorCO2(nn.Module):
"""
CO2 Scenario Surrogate:
Input: sequence of CO2(t) (batch, L, 1)
Output: sequence of Temp(t) (batch, L, 1)
"""
def __init__(self, hidden_size=64, num_layers=2):
super().__init__()
self.lstm = nn.LSTM(
input_size=1,
hidden_size=hidden_size,
num_layers=num_layers,
batch_first=True
)
self.fc = nn.Linear(hidden_size, 1)
def forward(self, x):
# x: (batch, L, 1)
out, _ = self.lstm(x) # (batch, L, hidden)
y_hat = self.fc(out) # (batch, L, 1)
return y_hat
model = ClimateEmulatorCO2().to(DEVICE)
optimizer = torch.optim.Adam(model.parameters(), lr=LR)
loss_fn = nn.MSELoss()
The model learns from decades of observed COββtemperature pairs.
Training the Surrogate
We train the model using mean squared error (MSE) loss:
for epoch in range(EPOCHS):
model.train()
train_loss = 0.0
for x_batch, y_batch in train_loader:
x_batch = x_batch.to(DEVICE)
y_batch = y_batch.to(DEVICE)
optimizer.zero_grad()
y_pred = model(x_batch)
loss = loss_fn(y_pred, y_batch)
loss.backward()
optimizer.step()
train_loss += loss.item() * x_batch.size(0)
train_loss /= len(train_loader.dataset)
# Simple test loss
model.eval()
test_loss = 0.0
with torch.no_grad():
for x_batch, y_batch in test_loader:
x_batch = x_batch.to(DEVICE)
y_batch = y_batch.to(DEVICE)
y_pred = model(x_batch)
loss = loss_fn(y_pred, y_batch)
test_loss += loss.item() * x_batch.size(0)
test_loss /= len(test_loader.dataset)
print(f"Epoch {epoch+1:03d} | Train Loss: {train_loss:.6f} | Test Loss: {test_loss:.6f}")
The trained surrogate captures the long-term warming trend driven by COβ.
COβ Scenario Emulator
Using the trained surrogate, we define several COβ scenarios:
- Stabilization Scenario
- Low-Growth Scenario
- Medium-Growth Scenario
- High-Growth Scenario
The surrogate predicts the temperature trajectory under each future COβ pathway.

Figure 6.7. Global COβ concentration and climate emulator temperature response under different future scenarios.
(A) Observed COβ concentration (solid black) and four illustrative future COβ pathways (dashed colored lines).
(B) Observed global mean temperature anomaly (solid black) and surrogate-predicted temperature responses (solid colored lines) under the same COβ pathways.
The figure demonstrates how different COβ trajectories produce distinct temperature outcomes in the surrogate model.
Summary
This chapter demonstrates how to use neural networks as surrogates [4, 27] for scientific processes. Using real COβ [28] and temperature data [29], we trained a surrogate model that can instantly estimate the temperature response to different COβ scenarios.
Note:
This surrogate is a simplified teaching demonstration.
Real relationships between COβ and temperature involve many additional forcings, including aerosols, methane, volcanic activity, solar variability, and internal climate cycles. A full climate model is required to capture these effects accurately [30].
Part IV: Code Optimization with AI
Vectorization Optimization
AI can transform slow, loop-based code into fast vectorized operations using NumPy [31]:
# Original slow code
def slow_distance_matrix(points):
"""Slow: nested Python loops"""
n = len(points)
distances = [[0.0] * n for _ in range(n)]
for i in range(n):
for j in range(n):
dx = points[i][0] - points[j][0]
dy = points[i][1] - points[j][1]
distances[i][j] = (dx**2 + dy**2)**0.5
return distances
# AI-optimized version
import numpy as np
def fast_distance_matrix(points):
"""Fast: NumPy broadcasting"""
points = np.asarray(points)
# Broadcasting: (n, 1, 2) - (1, n, 2) = (n, n, 2)
diff = points[:, np.newaxis, :] - points[np.newaxis, :, :]
# Euclidean distance
distances = np.sqrt((diff ** 2).sum(axis=-1))
return distances
# Benchmark
import time
n_points = 1000
test_points = np.random.rand(n_points, 2).tolist()
# Slow version
start = time.time()
slow_result = slow_distance_matrix(test_points)
slow_time = time.time() - start
# Fast version
test_points_np = np.array(test_points)
start = time.time()
fast_result = fast_distance_matrix(test_points_np)
fast_time = time.time() - start
print(f"Slow version: {slow_time*1000:.1f} ms")
print(f"Fast version: {fast_time*1000:.1f} ms")
print(f"Speedup: {slow_time/fast_time:.1f}Γ")
Expected Output:
Slow version: 1834.5 ms
Fast version: 15.0 ms
Speedup: 122.4Γ
Additional Optimization Examples
# Example 2: Moving average optimization
def slow_moving_average(data, window):
"""Slow: explicit loop"""
result = []
for i in range(len(data) - window + 1):
result.append(sum(data[i:i+window]) / window)
return result
def fast_moving_average(data, window):
"""Fast: NumPy convolution"""
return np.convolve(data, np.ones(window)/window, mode='valid')
# Benchmark
data = np.random.randn(10000)
window = 50
start = time.time()
slow_ma = slow_moving_average(data.tolist(), window)
slow_time = time.time() - start
start = time.time()
fast_ma = fast_moving_average(data, window)
fast_time = time.time() - start
print(f"\nMoving average:")
print(f"Slow: {slow_time*1000:.1f} ms")
print(f"Fast: {fast_time*1000:.1f} ms")
print(f"Speedup: {slow_time/fast_time:.1f}Γ")
# Expected: ~197Γ speedup
Output:
==================================================
EXAMPLE 2: MOVING AVERAGE OPTIMIZATION
==================================================
Before (loop): 3.644 seconds (estimated)
After (convolution): 0.0209 seconds
Speedup: 174.7Γ
==================================================
Excample 3 CORRELATION MATRIX OPTIMIZATION
# Generate data
n_features = 100
n_samples_corr = 10000
data_corr = np.random.randn(n_samples_corr, n_features)
# SLOW VERSION (nested loops)
def correlation_matrix_slow(data):
n = data.shape[1]
corr = np.zeros((n, n))
for i in range(n):
for j in range(n):
if i == j:
corr[i, j] = 1.0
else:
corr[i, j] = np.corrcoef(data[:, i], data[:, j])[0, 1]
return corr
# FAST VERSION (NumPy)
def correlation_matrix_fast(data):
return np.corrcoef(data.T)
# Benchmark
start = time.time()
_ = correlation_matrix_slow(data_corr)
slow_time = time.time() - start
start = time.time()
_ = correlation_matrix_fast(data_corr)
fast_time = time.time() - start
speedup3 = slow_time / fast_time

Part V: Automated Test Generation
Generating Comprehensive Tests
AI can automatically generate test suites from function code using pytest [32]:
def generate_tests_for_function(function_code):
"""Generate pytest unit tests"""
prompt = f"""Generate pytest unit tests for this function:
```python
{function_code}
Include tests for:
- Normal cases
- Edge cases
- Error handling
- Input validation
Tests:
# ... API call ...
return test_code
# Example function to test
function = """
def calculate_correlation(x, y, method='pearson'):
'''Calculate correlation between two arrays'''
import numpy as np
from scipy.stats import spearmanr
if len(x) != len(y):
raise ValueError("Arrays must have same length")
if method == 'pearson':
return np.corrcoef(x, y)[0, 1]
elif method == 'spearman':
return spearmanr(x, y)[0]
else:
raise ValueError(f"Unknown method: {method}")
tests = generate_tests_for_function(function)
**Generated Tests:**
```python
import pytest
import numpy as np
from your_module import calculate_correlation
class TestCalculateCorrelation:
"""Test suite for calculate_correlation function"""
def test_pearson_perfect_correlation(self):
"""Test perfect positive correlation"""
x = np.array([1, 2, 3, 4, 5])
y = np.array([2, 4, 6, 8, 10])
result = calculate_correlation(x, y, method='pearson')
assert np.isclose(result, 1.0)
def test_pearson_no_correlation(self):
"""Test zero correlation"""
x = np.array([1, 2, 3, 4, 5])
y = np.array([1, 1, 1, 1, 1])
result = calculate_correlation(x, y, method='pearson')
assert np.isnan(result) # Constant array has undefined correlation
def test_spearman_correlation(self):
"""Test Spearman correlation"""
x = np.array([1, 2, 3, 4, 5])
y = np.array([5, 6, 7, 8, 7])
result = calculate_correlation(x, y, method='spearman')
assert -1 <= result <= 1
def test_different_lengths_raises_error(self):
"""Test that different length arrays raise ValueError"""
x = np.array([1, 2, 3])
y = np.array([1, 2])
with pytest.raises(ValueError, match="same length"):
calculate_correlation(x, y)
def test_unknown_method_raises_error(self):
"""Test that unknown method raises ValueError"""
x = np.array([1, 2, 3])
y = np.array([4, 5, 6])
with pytest.raises(ValueError, match="Unknown method"):
calculate_correlation(x, y, method='kendall')
def test_empty_arrays(self):
"""Test behavior with empty arrays"""
x = np.array([])
y = np.array([])
with pytest.raises((ValueError, IndexError)):
calculate_correlation(x, y)
@pytest.mark.parametrize("method", ['pearson', 'spearman'])
def test_both_methods_return_valid_range(self, method):
"""Test that both methods return values in [-1, 1]"""
np.random.seed(42)
x = np.random.randn(100)
y = np.random.randn(100)
result = calculate_correlation(x, y, method=method)
assert -1 <= result <= 1
Summary
Physics-Informed AI transforms scientific computing by embedding physical laws into neural networks and accelerating simulations:
Physics-Informed Neural Networks (PINNs) [1, 2, 3]: Embed physical laws directly into neural architectures, enabling data-efficient, physics-consistent solutions to differential equations. Our implementations achieved:
- Heat equation PINN: RMSE of 0.002307 in 0.4 minutes
- Navier-Stokes PINN [15]: Sub-percent errors for velocity and pressure fields
- Atmospheric PINN [18, 19]: Correct physical profiles while respecting conservation laws
Loss Function Design: The composite loss structure balances physics constraints with data fitting. Key insights:
- Weight boundary/initial conditions (10Γ) to enforce constraint hierarchy
- Consider adaptive weighting for complex multi-physics problems
- Monitor divergence between physics and data losses to detect overfitting
Ablation Studies: Separating physics and data contributions reveals:
- Physics-only: Satisfies PDEs but may not match specific boundary conditions (RMSE ~4Γ10β»Β²)
- Data-only: Fits observations but violates physics between points (high PDE residual)
- Combined: Best accuracy AND physical consistency (RMSE ~2Γ10β»Β³)
Overfitting Considerations: PINNs can overfit despite physics constraints due to:
- Finite collocation points allowing violations between samples
- Data concentration in certain regions
- Loss weight imbalance favoring data over physics Mitigation strategies include train/val/test splitting, early stopping, regularization, and comprehensive validation checking both accuracy and physical consistency.
Simulation Surrogates [4, 27]: Replace expensive simulations with fast neural network approximations, enabling rapid scenario exploration. Our example achieved 3282Γ speedup with RΒ² of 0.978, demonstrating production-ready accuracy for parameter sweeps and uncertainty quantification [33].
Code Optimization [31]: Identify bottlenecks and generate vectorized, high-performance code automatically. Typical speedups of 100-200Γ for common scientific computing operations through vectorization, JIT compilation, and algorithmic improvements.
Testing and Validation [32]: Automatically generate comprehensive test suites and performance profiles ensuring correctness and reliability of physics-informed models.
Key Principles:
- Understand the Physics: PINNs and surrogates must respect domain constraints and conservation laws [7, 16]
- Design Loss Functions Carefully: Balance physics and data terms, consider adaptive weighting
- Validate Rigorously: Test against analytical solutions, monitor physics residuals, check physical bounds [16]
- Watch for Overfitting: Data-physics divergence, poor generalization, physical bound violations
- Quantify Uncertainty: Provide confidence estimates for predictions [33, 34]
- Benchmark Performance: Verify speedups and accuracy against traditional methods
- Start Simple: Begin with well-understood test cases before complex applications
Demonstrated Results:
| Component | Metric | Result | Status |
|---|---|---|---|
| Heat Equation PINN | RMSE vs analytical | 0.002307 | β Excellent |
| Heat Equation PINN | Training time | 0.4 minutes | β Fast |
| Navier-Stokes PINN | Velocity RMSE | 2.7e-3 | β Excellent |
| Navier-Stokes PINN | Pressure RMSE | 1.7e-3 | β Excellent |
| Navier-Stokes Ablation | Combined vs Physics-only | 94.5% improvement | β Data contribution verified |
| Atmospheric PINN | Physical profiles | Correct structure | β Verified |
| Surrogate Model | RΒ² Score | 0.978 | β Good |
| Surrogate Model | Speedup | 3282Γ | β Excellent |
| Code Optimization | Average speedup | 175.7Γ | β Excellent |
When to Use Each Approach:
PINNs are ideal when [2, 3, 7]:
- Physical laws are known (PDEs)
- Data is limited or expensive
- Physics consistency is critical
- Inverse problems need solving
- Boundary conditions are complex
Surrogates excel when [4, 27]:
- Expensive simulations exist
- Many parameter combinations needed
- Real-time predictions required
- Uncertainty quantification matters
- Optimization loops are computational bottlenecks
Hybrid approaches work best when [6]:
- Physics is partially known
- Both simulation and experimental data exist
- High accuracy with physics constraints required
The goal is not to replace traditional simulation [35] but to accelerate itβenabling researchers to explore parameter spaces, perform uncertainty quantification [33, 34], and make real-time predictions while maintaining physical consistency and scientific rigor [36, 37].
Next β Chapter 7: Domain Applicationsβexploring generative AI across chemistry, biology, physics, geoscience, and medicine with detailed case studies.
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Additional Resources
Software Libraries:
- DeepXDE: https://github.com/lululxvi/deepxde - PINN library for PDEs
- NeuralPDE.jl: https://github.com/SciML/NeuralPDE.jl - Julia PINN package
- JAX: https://github.com/google/jax - High-performance numerical computing
- scikit-learn: https://scikit-learn.org/ - Machine learning in Python
- NumPy: https://numpy.org/ - Array programming
- SciPy: https://scipy.org/ - Scientific computing
Physics-Informed Learning:
- Physics-Informed ML Review: Karniadakis et al. (2021)
- PINN Tutorial: https://github.com/maziarraissi/PINNs
- Neural Operator Tutorial: https://zongyi-li.github.io/blog/2020/fourier-pde/
Climate Data:
- ERA5 Reanalysis: https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era5
- NOAA Climate Data: https://www.ncdc.noaa.gov/
- NASA GISTEMP: https://data.giss.nasa.gov/gistemp/ Textbooks:
- Karniadakis, G. E., & Kirby, R. M. (2003). Parallel scientific computing in C++ and MPI. Cambridge University Press.
- Durran, D. R. (2010). Numerical methods for fluid dynamics. Springer.
- Strogatz, S. H. (2018). Nonlinear dynamics and chaos. CRC Press.
Recent Surveys:
- Cuomo et al. (2022). Scientific machine learning through PINNs
- Cai et al. (2022). PINNs for fluid mechanics
- Psaros et al. (2023). Uncertainty quantification in scientific ML
*Next β Chapter 7: Domain Applications in Chemistry, Biology, Physics and Geoscience *