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Click on a section of the interactive image map to go to its help information or scroll down to the corresponding section.

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Emitters

 

Emitter objects are used to simulate point-like radiation sources that interact with the extended objects in the model. Currently, only blackbody emitters are supported.

Create emitters just like any other Primitive Object after activating the emitter icon:

emitter icon

To edit the properties of the emitter select Emitters in the object type drop-down menu at the top of the Object Properties panel.

The emitters with their names appear in a list at the top. Select one to change its properties or remove it (click the Remove button) .

You set size of the emitter icon in the 3D views using the Mesh Radius text field. This size is only relevant for the visualization of the emitter in the viewport. It has no physical meaning.

The Visible button controls whether the emitter is used or not in the model. When you enable the Render button, the emitter will be included in the rendering. Note, however, that it is added on top of the image, i.e. as if the surrounding medium was transparent. This is also for visualization only.

To include the emitter more realistically in the rendering, you can model it as a small spherical dust sphere emitting at the appropriate temperature. Since the size of such a sphere will be near the resolution limit of the 3D volume grid, the accuracy of the emission values will be limited. Make sure that this is adequate for your application.

You can place the emitters anywhere in space by adjusting the position values in cartesian coordinates (xPos, yPos, zPos).

The physical properties of the blackbody model for the emitter can be set in terms of Temperature in Kelvin and the Radius in meters. The bolometric luminosity L in Watts is automatically displayed. When you "lock" the luminosity and then change either the temperature or the radius, the other parameter will be adjusted automatically to maintain the luminosity.

The Black Body Curve button opens a graph that shows the spectrum of the emitter within the range of the wavelengths set in the Render Module (see below). It shows additional useful physical quantities.

The emitter graph shows the spectral distribution of the theoretical blackbody.

emitter parameters

The emitter surface values of flux F, bolometric luminosity L, the number of ionizing photons beyond the Lyman limit Nu and the wavelength of the maximum λmax are displayed in the column on the right.

In the middle similar values are shown as obtained directly from the numerical emitter in the model.

Note that only the range is shown for the curve that is applied in the Transfer Renderer panel of the Render Module. The same range is used to calculate the model values. Therefore, when you do ionization calculations, make sure that the wavelength range in the renderer is adequate, i.e. the lower limit should be at or near zero.

When the Lyman Limit button is enables, an orange vertical line is show at the position of the Lyman limit.


emitter graph

 

   
 
   
  frame icon 16-Jun-2010  
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