Raster Solar Radiation (Spatial Analyst Tools)
Summary
Calculates the incoming solar insolation for every raster cell of a digital surface model for Earth or the Moon.
Solar insolation is calculated as the amount of solar radiation energy received per unit area during an amount of time and is measured in units, kilowatt hours per square meter (kWh/m2).
Usage
Calculating insolation can be computationally intensive for large data extents and when calculating many time intervals. This may require a lot of computing power and hard disk space. You can perform preliminary runs with data at a coarser resolution or a subset of the data to ensure that the settings are correct before committing a run with the full-resolution data.
The defined spatial reference of the Input surface raster parameter specifies whether the analysis will be for Earth or the Moon.
The solar radiation computation requires the Output Coordinate System environment value to be in a projected coordinate system (PCS). It is recommended that the data be in a PCS with units of meters. If you run the analysis with a spherical coordinate system, you must set the Output Coordinate System environment to a valid PCS.
When the input raster needs to be resampled, the bilinear technique will be used. An example of when an input raster may be resampled is when the output coordinate system, extent, or cell size is different from that of the input.
Daylight saving time is supported for Earth only. For the Moon, times must be specified in UTC.
The End date and time parameter value must be equal to or greater than the start date. The total span of time must not be greater than one year. The start and end date times can cross the calendar year.
Output radiation values will be calculated for each respective time interval. If no solar radiation was received for a time interval, the result for that location will have a value of zero.
If the total time specified between the start and end times is not equally divisible by the time interval, the total duration will be extended internally to provide the required number of time slices. For example, if the Time Interval parameter is set to cover three days but the difference between the specified start and end times covers eight days, the time interval will be extended to nine days. No partial results for times will be returned.
The minimum time interval for Earth data is 30 minutes and must be proportional to 30. The minimum time interval for Moon data is two hours and must be proportional to 2.
Use the Input analysis mask parameter (
in_analysis_maskin Python) to limit the output raster to only the locations or cells defined by the mask area. Additionally, it is important to consider the effect of the surface outside your area of interest. The mask can be defined by raster or feature data.The analysis mask does not affect the analysis extent used for calculations. This means that the topography or potential obstructions outside the mask area will influence the solar radiation values that are calculated for the defined areas.
If the mask input is a feature dataset, it will be converted to a raster internally using the cell size and cell alignment from the input surface raster value by default.
Specifying precomputed slope and aspect rasters as input will improve performance, especially if the tool will be run repeatedly or when analyzing larger datasets. If either the input slope or aspect raster values are not provided, values will be calculated from the input surface raster.
The Neighborhood Distance (
neighborhood_distancein Python) parameter determines the neighborhood size and calculates the surface parameter over this distance from the target cell center. The value cannot be less than the input raster cell size.A small neighborhood distance captures more local variability in the landscape, such as characteristics of smaller landscape features. With high-resolution elevation data, larger distances may be more appropriate.
If the Use adaptive neighborhood parameter is checked (
use_adaptive_neighborhood = "ADAPTIVE_NEIGHBORHOOD"in Python), the neighborhood distance will change with variability in the terrain. The neighborhood distance will shrink if there is too much variability in the calculation window.Earth's Moon does not have an atmosphere; the radiation parameters diffuse proportion and transmittivity are not relevant during analysis. As a result, the incoming diffuse solar radiation is zero and the total radiation is equal to direct solar radiation.
The diffuse proportion is the fraction of global normal radiation flux that is diffuse. Values range from 0 to 1. Set this value according to atmospheric conditions. Typical values are 0.2 for very clear sky conditions and 0.3 for generally clear sky conditions.
Transmittivity is the ratio of the energy reaching Earth's surface to that which is received at the upper limit of the atmosphere. Values range from 0 (no transmission) to 1 (complete transmission). Typically observed values are 0.6 or 0.7 for very clear sky conditions and 0.5 for a generally clear sky.
Transmittivity has an inverse relationship with the diffuse proportion parameter. Altering these values may affect the model result. Identifying the best values for the area of interest depends on several variables (such as location and time). You can change these values to compare how they affect the result.
The Sun Map Grid Level parameter controls the speed and accuracy of the computation. It adjusts the resolution of the hexagonal grid cells that will be used for the internal calculations, based on the H3 geospatial indexing system.
A lower grid level creates fewer larger sun map areas and decreases tool run time. A higher grid level creates more smaller sun maps, improving the accuracy of the result.
Valid values of the sun map grid level for Earth range from 5 to 7. For the Moon, the valid value range is from 4 to 6.
The default level is determined by the input surface raster. When analyzing surface data on Earth, if the analysis cell size is less than or equal to 4 meters, the default grid level is 6. If the cell size is greater than 4 meters, the default grid level is 5. For analyzing surface data on the Moon, the default level is 6.
The following table shows the average area of the hexagon grid cells for each sun map level, in units of square kilometers:
Level
Earth
Moon
4
Not applicable
131.6
5
252.9 (default > 4m)
18.8
6
36.1 (default < 4m)
2.69 (default)
7
5.16
Not applicable
This tool can be GPU accelerated, which means that if a compatible graphics processing unit (GPU) is available on your system, it will be used to enhance the performance of the tool. Use the Target device for analysis parameter (
analysis_target_devicein Python) to control whether the GPU or CPU will be used to run the tool.See GPU processing with Spatial Analyst for details on compatible GPUs, configuring and working with GPU devices, as well as troubleshooting tips.
When the output raster format is
.crf, this tool supports the Pyramid raster storage environment. Pyramids will be created in the output by default. For any other output format, this environment is not supported, and pyramids will not be created.See Analysis environments and Spatial Analyst for additional details on the geoprocessing environments that apply to this tool.
Additional resources:
Acton, Charles A. 1996. "Ancillary data services of NASA's Navigation and Ancillary Information Facility." Planetary and Space Science Volume 44, Issue 1, January 1996, pp. 65–70. https://doi.org/10.1016/0032-0633(95)00107-7
Acton, Charles, Nathaniel Bachman, Boris Semenov, and Edward Wright. 2018. "A look towards the future in the handling of space science mission geometry." Planetary and Space Science Volume 150, January 2018, pp. 9–12. https://doi.org/10.1016/j.pss.2017.02.013
Brodsky, Isaac. 2018. "Uber's Hexagonal Hierarchical Spatial Index H3." Engineering (blog), June 27, 2018. https://www.uber.com/blog/h3/
Parameters
| Label | Explanation | Data type |
|---|---|---|
|
Input Surface Raster |
The input elevation surface raster. |
Raster Layer |
|
Start Date and Time |
The start date and time for the analysis. |
Date |
|
End Date and Time |
The end date and time for the analysis. |
Date |
|
Input Analysis Mask (Optional) |
The input data that defines the locations where the analysis will occur. |
Composite Geodataset |
|
Input Slope Raster (Optional) |
The input slope raster that will be used when calculating the output solar radiation. If this input is not specified, the tool will calculate slope values internally from the input surface raster. Providing this value will improve performance, especially if the tool will be run repeatedly or when analyzing larger datasets. |
Raster Layer |
|
Input Aspect Raster (Optional) |
The input aspect raster that will be used when calculating the output solar radiation. If this input is not specified, the tool will calculate aspect values internally from the input surface raster. Providing this value will improve performance, especially if the tool will be run repeatedly or when analyzing larger datasets. |
Raster Layer |
|
Output Direct Radiation Raster (Optional) |
The output raster representing the direct incoming solar radiation value for each location. The output has units of kilowatt hours per square meter (kWh/m2). |
Raster Dataset |
|
Output Diffuse Radiation Raster (Optional) |
The output raster representing the incoming solar radiation that is diffused by the sky, layers of atmosphere, and other surroundings. The output has units of kilowatt hours per square meter (kWh/m2). |
Raster Dataset |
|
Output Direct Duration Raster (Optional) |
The output raster representing the duration of direct incoming solar radiation. The output has units of hours. |
Raster Dataset |
|
Time Zone (Optional) |
The time zone that will be used for the start and end time. The default is coordinated universal time (UTC).
|
String |
|
Adjust times for daylight saving time (Optional) |
Specifies whether the input time configuration will be adjusted for daylight saving time. This parameter is not applicable for analysis on the Moon.
|
Boolean |
|
Calculate insolation for time intervals (Optional) |
Specifies whether a single total insolation value will be calculated for the entire time configuration or multiple radiation values will be calculated for the specified interval.
|
Boolean |
|
Time Interval Unit (Optional) |
Specifies the time unit that will be used for calculating solar radiation values over the entire time configuration. This parameter is only available when the Calculate insolation for time intervals parameter is checked.
|
String |
|
Time Interval (Optional) |
The value of the duration or time between intervals. The default value is dependent on the interval unit specified. The default value for each of the available units are listed below.
|
Long |
|
Neighborhood Distance (Optional) |
The distance from the target cell center for which the output insolation value will be calculated. It determines the size of the neighborhood. The default value is the input surface raster cell size, resulting in a 3 by 3 neighborhood. |
Linear Unit |
|
Use adaptive neighborhood (Optional) |
Specifies whether neighborhood distance will vary with landscape changes (adaptive). The maximum distance is determined by the neighborhood distance. The minimum distance is the input raster cell size.
|
Boolean |
|
Diffuse Model Type (Optional) |
Specifies the type of diffuse radiation model that will be used.
|
String |
|
Diffuse Proportion (Optional) |
The proportion of global normal radiation flux that is diffuse. Values range from 0 to 1. Set this value according to atmospheric conditions. The default value is 0.3 for generally clear sky conditions. |
Double |
|
Transmittivity (Optional) |
The fraction of radiation that passes through the atmosphere (averaged overall wavelengths). Values range from 0 (no transmission) to 1 (all transmission). The default is 0.5 for a generally clear sky. |
Double |
|
Target Device for Analysis (Optional) |
Specifies the device that will be used to perform the calculation.
|
String |
|
Sun Map Grid Level (Optional) |
The resolution that will be used to generate the H3 hexagonal grid cells used for internal calculations. A lower grid level value creates fewer, larger sun map areas and decreases tool run time. A higher grid level creates more smaller sun maps improving the accuracy of the result. Valid values of the sun map grid level for Earth range from 5 to 7. For the Moon, the valid value range is from 4 to 6. By default, the grid level is determined by the input surface raster. When analyzing surface data on Earth, if the analysis cell size is less than or equal to 4 meters, the default grid level is 6. If the analysis cell size is greater than 4 meters, the default grid level is 5. For analyzing surface data on the Moon, the default grid level is 6. |
Long |
Return value
| Label | Explanation | Data type |
|---|---|---|
|
Output Solar Radiation Raster |
The output raster representing the total amount of solar radiation received per unit area across the input surface. The output has units of kilowatt hours per square meter (kWh/m2). |
Raster |
Environments
Cell Size, Cell Size Projection Method, Current Workspace, Adjust for Daylight Saving, Extent, Geographic Transformations, GPU ID, Mask, Output Coordinate System, Parallel Processing Factor, Processor Type, Pyramid, Scratch Workspace, Snap Raster, Time Zone
Licensing information
- Basic: Requires Spatial Analyst
- Standard: Requires Spatial Analyst
- Advanced: Requires Spatial Analyst