- Functions compatible with TRISCO v14.0w: recalculation of blocks (Blocks > Arrange Blocks); clip blocks (Blocks > Reduce to Clip); detect void space (Blocks > Convert Void to Blocks); show materials as transparent blocks (Image > Show Transparent), display grid unit; simulation of adiabatic surface of transparent material (type TRANSMAT), graphic output of single isothermal line.
- Show north direction and sun paths (function Image > Show North from main menu) and sun position (function View > Sun Position from graphic output window).
- Controls which allow to replace boundary condition functions (temperature, heat power, heat flux, heat transfer coefficient, ventilation) or material property functions (thermal conductivity, infrared emissivity, solar reflection factor, solar transmission factor) with other functions (of the same type), dependent on the temperature in a sensor node compared to a temperature target function (of time) and desired heating or cooling.
The replacement of a ventilation function can also be dependent on a minimum required temperature difference between two ventilation zones.
- Control functions can also refer to constant functions.
The constant function is reintroduced as function type in the Functions window.
- The infrared emissivity of a material surface and the solar transmission factor of a material can be a function of time (intended for use with controls, e.g. for the simulation of solar screens).
- Default data file Voltra.vtr with initialisation values for thermal properties per colour.
- Time dependent functions for thermal conductivity, total surface heat transfer coefficient and convective heat transfer coefficient.
- Functions compatible with TRISCO v12.0w: automatic split for grid refinement;
equivalent thermal conductivities for cavities with different surface emissivities.
- Show temperature or heat flux under the cursor in the graphic output.
- 3D visualisation of sun position at any time step.
- Show temperature profile along a grid line at any time step.
- Improved more stable calculation of systems with ventilation flows.
- Diffuse solar reflection also possible in solar zone (of type BC_SKY).
- Sun obstacles (as in CAPSOL and BISTRA), defined as sky hemisphere regions, which block direct solar radiation and decrease diffuse solar irradiation.
- Import BISTRA data.
- Solar processor adapted to use of 2D geometries (SECTRA).
- Adjust coordinates of output nodes and output blocks after any grid operation.
Contains 3D solar processor
Same solar radiation climate data files as in CAPSOL (global and diffuse radiation on a horizontal surface).
Input required of north orientation.
Calculation of sun position and visualization of shadows cast by direct sun light.
Creation of AVI animation file of shadows over calculation period.
Additional material properties required: reflection factor (may be a function of the angle of incidence), transmission factor (to indicate a transparent material).
Calculation and visualization of absorbed solar fluxes on material surfaces due to solar radiation.
Direct solar radiation on an exterior material surface depends on geographical location, solar radiation climate data, day of year, clock time, surface orientation.
Diffuse solar radiation on an exterior material surface depends on the view factor to the open sky and is calculated using Muneer's radiation model (also used in CAPSOL).
Reflected radiation (of direct and diffuse incident radiation) at an exterior material surface is lost (as in CAPSOL). An input parameter (ground reflection factor) allows to take into account the reflected radiation from the environment.
Radiation on transparent materials are transmitted to internal zones.
Direct radiation is projected on internal walls following the solar rays.
Diffuse radiation is distributed on all internal walls proportional to the view factors.
All reflected radiation at an interior material surface is diffuse and is redistributed to the other interior surfaces proportional to the view factors.
The scheme of successive internal reflections and transmissions is solved using a radiosity method.
The view factors can be obtained from a prior view factor calculation using a coarser grid (to speed up the processing time and reduce the required memory space).
The absorbed solar fluxes can be output to an AVI animation file or output to a text file.
The absorbed solar fluxes can be used as boundary conditions for a thermal simulation (calculation of temperatures). In this way solar heat gains on the thermal behaviour of a construction can be studied.
The format of view factor file is modified.