Physics-grade engineering studios · v2026.6

Solve the physics.Ship the engineering.

Aurora is the workspace for engineers who live inside the problem — acoustic, molecular, multiphysics. Validated solvers, manufacturer-verified equipment, and an inspector built around the daily loop of finding the answer.

Enter Aurora See the solvers
2
physics engines
141
microphones
107
loudspeakers
iterations
/ liveInside a running job
aurora.cloud / acoustics / spl-coverage · job 41A2

SPL coverage prediction

Hall A · 31 sources · 64 mics

+0.4 dB / step
20Hz200Hz2kHz20kHz

Worker class

GPU · A100 80GB · ×4

Runtime
00:42:18
Queue
Priority
Spend
$24.81
Est. total
$36.40
Progress68%
NeumannSchoepsDPASennheiserAKGMeyer Soundd&b audiotechnikL-AcousticsGenelecAdamsonShureBeyerdynamicEarthworksRoyerColesNeumannSchoepsDPASennheiserAKGMeyer Soundd&b audiotechnikL-AcousticsGenelecAdamsonShureBeyerdynamicEarthworksRoyerColes
/ 01Physics engines, shipped

Two engines live. More physics on the roadmap.

Browse all studios

Acoustic physics

Aurora Acoustics

Wave equation · ray tracing · image-source

141 microphones · 107 loudspeakers

Molecular physics

Aurora Nano

Molecular dynamics · structural analysis

Atomistic workspace installed

/ 01.5Inside Aurora Acoustics

Solver-grade inspector. For the engineer in the loop.

Polar response, RT60 decay, material absorption, and source coverage — every quantity traceable back to the wave equation and the manufacturer datasheet that produced it. The daily working tool, not a marketing surface.

  • Validated solvers — ray tracing, image-source, wave-based hybrid
  • Per-octave RT60 with material absorption breakdown
  • Diff two iterations side-by-side, frequency-by-frequency
inspector · neumann u87 · cardioid

Polar response

U87 · 2.4 kHz

90°

RT60 decay

Hall A · 1.84 s

125Hz1kHz8kHz

Absorption mix

α₅₀₀ = 0.42
Wood panel
48%
Stage curtain
28%
Audience seating
18%
Concrete shell
6%
/ 02Where your physics runs

Same engine. Three places to solve it.

The physics is identical whether the job runs on your laptop, a remote workstation, or a managed fleet. The infrastructure is plumbing — the engine is the point.

0 ms queue
01

Local

On your workstation

Run the studio entirely on the machine you're sitting at. Zero network, zero queue, full control. Ideal for iterative inspector work and quick what-ifs.

  • Native CPU / GPU
  • Offline capable
  • No spend meter
Hot in <30s
02

Online

Burst to a remote workstation

Stream into a dedicated remote workstation when your laptop runs out of headroom. Same studio surface, larger silicon — billed by the second it's hot.

  • Dedicated RTX / Ada
  • Stream from anywhere
  • Per-second billing
Parallel ×N
03

Cloud

Elastic managed fleet

Fan out hundreds of parametric runs across the Aurora fleet. Pin a region, pick a worker class, watch every dollar settle per job before it ships.

  • A100 / H100 pools
  • Region pinning
  • Per-job spend caps
aurora.router · job spl-coverage · 7F12
LocalREADY
M-series · 32GB
OnlineSELECTED
RTX 6000 · 48GB
CloudQUEUED
A100 ×4 · eu-west-1
est. runtime · 42 minest. spend · $3.18selected · Online
/ 03Physics engines

Engines that match the problem you're solving.

Aurora is built around real physics, not generic dashboards. Every studio inherits the same engineer-first inspector, tuned to the equations of its domain.

Acoustic physics

From the wave equation to the room

Hybrid solvers — ray tracing, image-source, and wave-based — drive SPL coverage, source placement, and inspection. Every result traces back to the equation and the datasheet that produced it.

Molecular physics

Atoms, bonds, and dynamics

Aurora Nano brings molecular dynamics and structural analysis into the same engineer-first surface — geometry, force fields, and analysis side-by-side.

Verified equipment

Manufacturer-grade libraries

141 microphones, 107 loudspeakers, real frequency response and polar data sourced from manufacturer datasheets. The library grows with every studio.

aurora.cloud / fleet
A100-01
spl-coverage · 41A2
92%
eu-west-1
A100-02
ir-bake · 8C19
78%
eu-west-1
A100-03
polar-sweep · 22F0
64%
us-east-2
CPU-14
import · cad-mesh
22%
eu-west-1
A100-04
— awaiting queue
0%
us-east-2
spend · today$214.06
/ 03.5Inside cloud mode

Cloud mode. Honest spend.

When a job outgrows your local or online workstation, fan it out to the Aurora cloud fleet. Pin a region, pick a worker class, see the meter tick — no black-box billing, every dollar attributed to a job.

Regions
3 active
Worker classes
CPU · GPU · A100
p95 queue
42s
Budget alerts
Per project
/ 04The platform

An engineering platform, not a render farm.

Validated acoustic solvers

Ray tracing, image-source, and wave-based hybrid — chosen per frequency band, traceable back to the underlying physics.

Molecular dynamics

Aurora Nano: atomistic workspace, force fields, structural analysis. Engineer the molecule, not the toolchain.

Verified equipment libraries

Manufacturer datasheets ingested and validated — 141 microphones, 107 loudspeakers and counting.

Engineer-first inspector

Polar plots, decay curves, absorption breakdown — every quantity surfaced where the engineer is already looking.

Studio templates

Premium templates and presets inherit Aurora's dark technical interface — never starter scaffolding.

Team operations

Seat controls, roles, shared projects, activity traces, and clean technical handoff between engineers.

Run anywhere

Same engine, three targets — local workstation, online burst, or managed cloud fleet. Compute is plumbing.

Enterprise posture

Audit-ready settings, region planning, secure connectors, premium support — the boring stuff, done right.

/ 05Trusted by engineering teams

Built with the teams who run it.

Aurora replaced three legacy solvers and an internal toolchain. The acoustic engine actually agrees with the room — we stopped fighting our tools and started solving the problem.
Dr. Lena Hofmann
Head of Acoustic Engineering
Klang Systems · Munich
The equipment library alone is worth the seat — every mic and loudspeaker we use is already validated with manufacturer-grade polar and frequency data.
Marcus Aldridge
Principal Consultant
Aldridge Acoustics · London
We iterated SPL coverage 400 times in a weekend. The engine was right the first time; we spent the cycles on the engineering, not on convincing the solver.
Sofia Reyes
Simulation Lead
Volta Multiphysics · Barcelona
/ 06Pricing

Premium engineering seats. Honest compute.

You pay for the engine and the engineering surface. Cloud bursts and managed runs are metered separately — every job estimates its cost before it starts.

Pilot

$1,200
per seat / month

Cloud usage billed separately

  • Aurora Acoustics access
  • Equipment Library
  • Shared projects
  • Standard job queues
Request pilot
Most popular

Studio

$8,500
base / month

Includes seat pool · compute metered

  • Priority cloud queues
  • Aurora Nano installed
  • Team governance
  • Premium support
  • Region pinning
Book studio plan

Enterprise Cloud

Custom
annual platform agreement

Reserved capacity + usage controls

  • Dedicated regions
  • SSO & audit logs
  • Custom studio templates
  • Dedicated success engineer
  • 99.95% SLA
Talk to sales

Cloud spend varies by queue priority, worker class (CPU / GPU / High-memory), region, storage, and simulation runtime. Reserved capacity available on Enterprise.

/ 07FAQ

Questions, answered.

No. Aurora gives you three compute targets — local (your workstation), online (a dedicated remote workstation streamed to you), and cloud (a managed elastic fleet). The studio surface is identical; you pick the target per job based on size, urgency, and budget.

Bring the physics problem.
We brought the engineering.

Validated solvers. Manufacturer-verified equipment. An inspector built around the engineer in the loop — and compute that gets out of the way.