Power is an application of Systema dedicated to compute in-orbit performances
The Power application is based on:
- An interactive schematic editor to build the power architecture with various elements such as solar arrays, batteries and regulators, taking into account electrical and thermal aspects
- The computation of external fluxes and radiative couplings (with geometrical model and mission definition)
- The Thermisol solver, which is a coupled thermal power solver, to compute the electrical and thermal behaviour of the system
It is a complete solution to compute the in-orbit electrical performances of an architecture:
- Possibility to create a geometrical model and define a mission to compute the external fluxes and radiative couplings
- Geometrical (thermal) model and electrical architecture can be linked via thermal node numbers
- A coupled thermal power solver allows to perform complete analyses taking into account thermal aspects due to space environment
An interactive Schematic editor:
- An editor to build the electrical architecture
- Set of generic components are provided with the application: solar array, battery, regulator, iode, resistance, power load, capacitance
- Combine electrical, thermal and logical networks of components
Component editor:
- An editor to build the electrical architecture
- Set of generic components are provided with the application: solar array, battery, regulator, diode, resistance, power load, capacitance
- Combine electrical, thermal and logical networks of components
- User can program his own components using MORTRAN and C and reuse them for further analyses via the Graphical User Interface
Systema-Power embeds all the possibilities of Systema-Thermica to feed the power analysis:
- Radiative exchange factors computation module based on an multi-threaded ray-tracing algorithm It allows handling realistic thermo-optical properties:
- Absorptivity / emissivity
- Specular / diffuse reflection
- Specular / diffuse transmission
- Refractive index
- Solar & planets fluxes:
- Computed as function of the position of the Sun
- Efficient ray-tracing algorithm
- Planet (or moon) IR and albedo fluxes