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10. Sky View Factors10.1. Calculating the Sky View Factor¶The Sky View Factor (SVF) is used in the evaluation of the impact of urban geometry on the micro-climate, specifically temperature and the Urban Heat Island phenomenon. Sky View Factors help in the comprehension of an area’s potential direct sunlight in a given amount of time. The SVF indicates the ratio between : the radiation received / emitted by a surface from/to the skyand the theoretical total hemispheric radiating environment.Direct “visibility” between the sky and a plane means radiation can escape the urban setting into the atmosphere, whereas radiation between said plane and another plane keeps radiation trapped. Higher SVFs therefore indicate spaces that would theoretically cool down (emit more radiation towards the sky) than a space with low SVF.Let’s see how we assess the Sky View Factor in an urban setting. First off, follow the instructions to create a grid layout of the urban space. For this example, we’re using a 10x10 grid, with z=0.1m.Next, select the Sky View Factor in the BatchProcessing options.See alsoSampling the Bounding boxBatch ProcessingFill in the next two command boxes accordingly. In the first box: Select SkyViewFactor as process Select the layer containing your sampled bounding box Select “Sketchup:Face”The second command allows you to control the SVF parameters: Select the number of rays used to calculated the SVF, ie: its precision. Be careful though, this process is repeated for each sample and will impact your computing time dramatically Set the z0 value to 0.1, meaning we will check the SVF at ground level. Select your unit length Finally, select the name under which the values are stored. We recommend you keep  the default name “svf” to keep from any confusion.Once that is done, you can check your new feature by selecting Extensions &#62; View &#62; PickUpEntity  to view individual squares, or by going to Extensions &#62; View &#62; PrintAttributeValues ** and by selecting **svf:Float in the following command box to show the values of every sample.But there is a much better way of viewing and presenting the data, much like what we’ve done when viewing building heights.See alsovisualizing building heightsSelect Extensions &#62; t4su &#62; View &#62; ColorFaces. In the next command box, select the color range you wish to use. In the drop-down menu next to “select attribute’s name”, find and select “svf:Float” Select the number of classes you want for your map. Hit OKYour grid should be colored to resemble something like this :Sky View Factor over Cathedral Sector, NantesAssociated Legend of the SVF Map.Unless you’ve taken a color range with a “-” in front, lighter values express areas with a high SVF, meaning areas which “view” much of the sky. Darker areas, mostly in small streets and inside building blocks, do not “see” much sky directly : most of the radiation is captured and recaptured by adjacent walls.&#160;10.2. Sun View Factors¶Once you’ve created a Sun Path, you can use it to calculate the Sun View Factor, which works a little like the Sky View Factor : instead of checking covisibilities between geometry faces and the sky dome, it will check the covisibility between a geometry and each point of your Sun Path.See alsoDrawing Sun PathsCalculating the Sky View FactorClicking on Extensions &#62; t4su &#62; Sun Views &#62;SunViewFactor will enable the following command box : Select the two corresponding layers : your SunPath layer and your geometry layer. You can choose to alerate the results slightly by choosing a specific type of sky (from “pure” to “cloudy”).Once that is done, you will find that your geometries now have extra attributes: directSolarIrradiance:Float,represents the cumulative theoretical radiative energy received by the geometry from the sun at each point, which depends on their  covisibility and the angle of the sun’s rays.* nbHitsTotal:Int,the number rays between the geometry and the SunPath points nbMinTotal:Float,the number of rays between the geometry and SunPath, multiplied by the frequency of the plot of the Sun Path (eg: for a plot every 5 minutes if nbHitsTotal=2, nbMinTotal=10) ratioTotal:FloatYou can then use ColorFaces to see the geographical variations of each of these new attributes. Below, we’ve drawn two different maps of the same phenomena : The number of minutes a defined space will receive direct sunlight on two opposing dates : 21st of June and 21st of December, the longest and shortest days of the year respectively.Number of Minutes of Sunlight for the 12st of DecemberNumber of Minutes of Sunlight for the 21st of JuneSee alsoViewing Direct Solar Irradiation along a PathBasic Example of Data VisualizationSampling the Bounding box