Orbital Debris Detectability
A forward model for detecting sub-centimetre orbital debris by its ionospheric plasma wake — drivable by a human or by an AI agent through the same controls.
Parameters
5 mm
10 km/s
400 km
Detectability
0
/ 100 at 400 km, daytime
illustrative model — not NASA's actual soliton simulation.
What's real here
Real
- The physics forward model runs in-page
- WebMCP tool registration (4 tools)
- Live deploy — one static file, no backend
Simplified
- Ionosphere data is hardcoded
- Closed-form terms, not a plasma solver
- No validation against observations
Next
- Real ionosphere data (IRI / GNSS TEC)
- A trained ML inverse model
- Multi-sensor localization