Creating an Intensity Sensor

This page shows how to create an Intensity Sensor that computes and analyzes radiant or luminous intensity.

To create an Intensity Sensor:

  1. From the Light Simulation tab, click Intensity .
  2. Set the Axis System of the sensor by clicking to select the origin, to define X axis and to define the Y axis or click and select a coordinate system to autofill the Axis System.
    Note: If you define manually one axis only, the other axis is automatically (and randomly) calculated by Speos in the 3D view. However, the other axis in the Definition panel may not correspond to the axis in the 3D view. Please refer to the axis in the 3D view.
    The rays are integrated on Z plane.
  3. If you want to import a template file to define the sensor, in XMPTemplateFile, click Browse to load an .xml file.
    Note: An XMP Template is an .xml file generated from an XMP result. It contains data and information related to the options of the XMP result (dimensions, type, wavelength and display properties).

    When using an XMP Template, measures are then automatically created in the new .xmp generated during the simulation based on the data contained in the template file.

    • If you want to inherit the axis system of the sensor from the XMP Template file, set Dimensions from file to True.

      The dimensions are inherited from the file and cannot be edited from the definition panel.

    • If you want to define the radiance sensor according to display settings (grid, scale etc.) of the XMP Template, set Display properties from file to True.

  4. In General, from the Type drop-down list:

    • Select Photometric if you want the sensor to consider the visible spectrum and get the results in cd.

      Note: In case of a photometric result generation, the International Commission on Illumination (CIE) defines the visible spectrum as follows: "There are no precise limits for the spectral range of visible radiation since they depend upon the amount of radiant flux reaching the retina and the responsivity of the observer. The lower limit is generally taken between 360 nm and 400 nm and the upper limit between 760 nm and 830 nm".

    • Select Radiometric if you want the sensor to consider the entire spectrum and get the results in W/sr.

      Note: With both Photometric and Radiometric types, the illuminance levels are displayed with a false color and you cannot make any spectral or color analysis on the results.
    • Select Colorimetric to get the color results without any spectral data or layer separation (in cd or W/sr).

    • Select Spectral to get the results and spectral data separated by wavelength (in cd or W/sr).

      Note: Spectral results take more time to compute as they contain more information.
  5. From the Format drop-down list, select XMP to integrate light according to a standard coordinate system.
  6. From the Orientation drop-down list, define which axis represents the polar axis:
    • Select X as meridian and Y as parallel to define X as the polar axis.

    • Select Y as meridian and X as parallel to define Y as the polar axis.

      Note: These orientations are often used for automotive regulations.

      X as meridian corresponds to the orientation of an IESNA B format

      Y as meridian corresponds to the orientation of an IESNA A format.

    • Select Conoscopic to take Z as the polar axis.
  7. From the Layer drop-down list:
    • Select None to get the simulation's results in one layer.

    • Select Source if you have created more than one source and want to include one layer per active source in the result.

      Tip: You can change the source's power or spectrum with the Virtual Lighting Controller in the Virtual Photometric Lab or in the Virtual Human Vision Lab.

    • Select Face to include one layer per surface selected in the result.

      Tip: Separating the result by face is useful when working on a reflector analysis.

      • In the 3D view click and select the contributing faces you want to include for layer separation.

        Tip: Select a group (Named Selection) to separate the result with one layer for all the faces contained in the group.

      • Select the filtering mode to use to store the results (in the *.xmp map):

      • Last Impact: with this mode, the ray is integrated in the layer of the last hit surface before hitting the sensor.

      • Intersected one time: with this mode, the ray is integrated in the layer of the last hit selected surface if the surface has been selected as a contributing face or the ray intersects it at least one time.

    • Select Sequence to include one layer per sequence in the result.

  8. Define the dimensions of the sensor on X and Y axes:




    • If you want to link the start and end points values, set Mirror extent to True.

    • Define the Start and End points of the sensor on X and Y axes by editing the values in degrees.

    • In Sampling, define the number of pixels of the XMP map.

      The Resolution is automatically calculated.

      Note: Speos supports a maximum resolution of 23170 * 23170 pixels.
  9. If you selected Colorimetric or Spectral as sensor type, in Wavelength, define the spectral range the sensor needs to consider:

    • Edit the Start (minimum wavelength) and End (maximum wavelength) values to determine the wavelength range to be considered by the sensor.

    • If needed, in Sampling, adjust the number of wavelengths to be computed during simulation.

      The Resolution is automatically computed according to the sampling and wavelength start and end values.

  10. If you want to bring the measuring field of the sensor closer to the source, in Properties set Near field to True.
    Note: If Near field is deactivated, the intensity is located at the infinite.

    The results obtained with a near-field sensor can be inaccurate on the edge of the map, over a width equal to the radius of a cell.

    1. In Cell Distance, define the position of the sensor in regard to the origin in the 3D view.
    2. In Cell Diameter, define the actual size of the photosensitive sensor.
      Make sure to define a Cell Diameter bigger than the pixel size. For more information refer to Near field.
  11. In Optional or advanced settings :

    • If needed, adjust the preview of the grid by editing the values.

    • If you want to adjust the position preview of the sensor, change the radius (in mm).

    • From Intensity result viewing direction, define where the sensor is placed regarding to the source:

      • Select From source looking at sensor to position the observer point from where light is emitted.

      • Select From sensor looking at source to position the observer in the opposite of light direction.

The intensity sensor is created and is visible both in Speos tree and in the 3D view.