MODELING & SIMULATION
Build a network, specify its properties and boundaries, and explore its solution.
Choose a solver below. All use your existing IICSM AI workspace username and password. A lock icon marks links that require sign-in.
HEAT TRANSFER
Model lumped thermal capacitance, conduction, prescribed convection, radiation, and applied heat sources with SINDA-style input.
FLUID FLOW & HEAT TRANSPORT
Specify connected fluid nodes and branches with SINDA-style input, or generate a Cartesian grid for 2D and 3D flow calculations.
SOLID MECHANICS
Define material properties, nodes, element connections, supports and forces with SINDA-like input.
QUANTUM AND CLASSICAL KINETICS
Direct Bose/Fermi binary collisions, classical discrete velocities and lattice collision / streaming, with 1D/2D/3D SINDA-like inputs.
REPRESENTATIVE PHYSICS MODELS
Confined-particle Schrodinger ground states with probability, energies and exact box solutions.
REPRESENTATIVE PHYSICS MODELS
Monatomic harmonic lattice vibrations, phonon dispersion and the continuum elastic-wave limit.
REPRESENTATIVE PHYSICS MODELS
Concentration diffusion and transverse shear-wave decay with analytical liquid transport solutions.
ELECTROMAGNETISM & PLASMA
Evolve small electron-density waves on a periodic 1D, 2D or 3D mesh. Compare a warm-fluid calculation with the Langmuir / Bohm–Gross dispersion relation.
ELECTROMAGNETISM & PLASMA
Solve 1D/2D/3D plasma MHD and collisionless Vlasov–Maxwell kinetics with SINDA-like nodes and conductors, coupled fields, velocity moments and Lawson energy-balance diagnostics.
ELECTROMAGNETISM & PLASMA
Solve the source-free vacuum Maxwell curl equations on periodic 1D, 2D and 3D grids. Inspect all six electromagnetic components, divergence constraints and wave energy.
ELECTROMAGNETISM & PLASMA
Build SPICE-style netlists for resistor, capacitor, inductor, independent source and diode networks. Run DC operating-point or zero-state transient analysis and inspect voltages and branch currents.
Build named models from all eleven solver categories. Prescribe SINDA-like connections between nodes, run native solvers, and inspect coupling results in one dedicated workspace.
Open all three editors. Exchange heat, map temperatures into thermal expansion, and apply fluid pressures to a solid. Load the 5×5 example with 25 nodes in each category.
These are independent educational solvers with SINDA-style input, not the complete NASA GFSSP or SINDA/FLUINT products. Results require independent validation and must not be the sole basis for safety-critical decisions. Tools and content are provided without a guarantee of accuracy, completeness, availability, or fitness for a particular purpose.