Sentinel-1 Intensity Analysis in ENVI SARscape Tutorial

This tutorial provides an introduction to working with Sentinel-1 synthetic aperture radar (SAR) data in ENVI® SARscape. You will learn about SAR remote sensing and how to prepare Sentinel-1 data for backscatter intensity analysis. Steps are provided for downloading data, importing data into SARscape, setting preferences, multilooking, spatial subsetting (sample selection), filtering, and geocoding. You will also learn how to create a color composite of intensity images.

The following software must be installed and licensed on your system:

See the following sections:

Files Used in This Tutorial

Sample data files for the tutorial are available from our ENVI Tutorials web page. Click the "SAR Getting Started" link under "ENVI Tutorial Data." Extract the data to a new directory on your local drive called SARGettingStarted. Make sure this directory has write permissions. Then create a subfolder called TempFiles.

File

Description

2017-12-12-SLC-Power/

Folder containing Sentinel-1 intensity (power) images of a region in Chile

StudySite.shp (and .dbf, .shx)

Shapefile indicating the boundary of the study area

You will also need to download a digital elevation model (DEM) for geocoding. The Geocode the Images section of this tutorial provides instructions for downloading an ASTER Global DEM or SRTM-3 V4 DEM.

Introduction to SAR

Synthetic aperture radar (SAR) is an active imaging system, whereby the sensor provides its own energy source to illuminate the Earth's surface. It emits microwave radiation toward the surface and receives the reflected signal. In contrast, optical sensors—such as Landsat, Sentinel-2, and WorldView—rely on the sun to illuminate the surface. They measure the amount of reflected sunlight at the sensor. Thus, optical sensors that measure visible to shortwave-infrared (SWIR) wavelengths can only provide useful images during the daytime. Cloud cover can obscure the surface for optical sensors, which severely limits the extraction of meaningful information about the surface. SAR sensors, on the other hand, can obtain measurements any time of day and in any cloud-cover condition.

SAR imaging is sensitive to the effects of topography, surface roughness, and moisture. This makes it suitable for a wide variety of scientific applications. The interactions between microwave sensing and the Earth's surface are complex. This, combined with the amount of processing involved, tends to discourage some users from working with SAR data. This tutorial provides an introduction to SAR remote sensing so that you can begin to explore its full potential.

Spaceborne and airborne radar systems transmit microwave pulses toward the Earth's surface in a side-looking (oblique) direction. The sensor's antenna focuses the regular pulses into a beam, which illuminates the surface at a right angle to the direction the sensor is moving. The direction of the antenna beam is called the range, or ground range. The direction of the flight path is called the azimuth.

Sentinel-1 transmits energy at a frequency of 5.405 GHz, in the microwave region called the C-band. In this region, microwave energy only partially penetrates through surfaces such as vegetation and soils, compared to L-band sensors that can penetrate all the way through those materials under dry conditions. (Moisture prevents the energy from penetrating through most soils.) X-band sensors are primarily used for investigations of surface features since the microwave energy only penetrates the top layer layer of materials.

The following figure shows the different SAR missions and their microwave regions. Click on the thumbnail to see a larger version.

The antenna receives a portion of the microwave energy reflected from the surface objects within the beam pattern. The ratio of the power between the transmitted and reflected energy is called backscatter.

Backscatter is dimensionless; however, it is typically reported in decibels (dB). Backscatter consists of two variables: amplitude and phase. Amplitude—also called magnitude—is a measure of the strength of the reflected signal at the sensor. Phase represents the point along the wave of the reflected signal when it is received at the sensor. The difference in phase between the transmitted signal and the received signal provides information about the surface. This difference is measured in radians or degrees.

The following diagram shows the relationship between amplitude and phase in a microwave signal:

Since the backscattered signal is a combination of two variables, that signal must be represented as a complex number for the purposes of creating a digital image. Thus, in an unprocessed radar image, each pixel represents a complex value that contains amplitude and phase information about the microwave field backscattered by all the scattering objects within the radar beam. The amplitude/magnitude is the real part of the complex value, while the phase is the imaginary part. Phase is more difficult for us to visualize, so that is why it is represented as the imaginary part.

The Sentinel-1 data used in this tutorial were acquired in Interferometric Wide swath (IW) mode. This is the primary acquisition mode over land, and it is the most frequently used mode for Sentinel-1 applications. See the Interferometric Wide Swath topic in the Sentinel-1 SAR User Guide for details.

For more detailed information about the physical processes involved with radar remote sensing, consult the references at the end of the tutorial.

In the next section, you will explore some of the tools available in ENVI SARscape for working with Sentinel-1 data.

Working with Sentinel-1 Data in ENVI SARscape

ENVI SARscape provides many different tools for importing and processing various radar formats. The SARscape folder in the ENVI Toolbox contains all of the available tools for the SARscape modules you have installed and licensed. Also included are options for setting preferences, performing administrative tasks, and reading the ENVI SARscape documentation provided by sarmap SA.

Given the large number of tools that are provided, knowing where to begin with Sentinel-1 data processing can be a challenge. This tutorial describes one specific workflow: preparing Sentinel-1 data for backscatter intensity analysis. The workflow involves the following steps:

Set ENVI Preferences

  1. Start ENVI.
  2. From the ENVI main menu bar, select File > Preferences.
  3. Click the Directories item on the left side of the Preferences dialog.
  4. Click inside the Input Directory field, then click the > button that appears. The Browse for Folder dialog appears.
  5. Navigate to the SARGettingStarted directory and click OK. You created this directory earlier in the Files Used in This Tutorial section.
  6. Click the > button next to Output Directory.
  7. Select the SARGettingStarted directory and click OK.
  8. Click the > button next to Temporary Directory.
  9. Navigate to the SARGettingStarted\TempFiles folder. Click OK in the Browse for Folder dialog.
  10. Click OK in the Preferences dialog.

Set SARscape Preferences

  1. In the ENVI Toolbox, select SARscape > Preferences > Preferences common. The Preferences [General] dialog appears.
  2. Select the Directories and batch file name item on the left side.
  3. Click inside the Working directory preference field, then click the > button. The Browse for Folder dialog appears.
  4. Select the SARGettingStarted\TempFiles directory. Log files and trace files from SARscape processes will be saved to this directory.

    5. Tip: You do not need to set the Sentinel-1 auxiliary directory preference for this tutorial. You would normally set this preference to a directory that contains precise or restituted orbit files, which are used for interferometry.

  5. Click Ok in the Preferences [General] dialog.
  6. In the ENVI Toolbox, double-click Preferences specific.
  7. Click the Load Preferences button in the Preferences dialog and select Sentinel TOPSAR.
  8. When prompted to load the Sentinel TOPSAR preferences, click Yes.
  9. Click Ok in the Preferences [Sentinel TOPSAR] dialog.

Tip: Be sure to set the specific preferences each time you start ENVI. This will automatically set the processing parameters that are optimized for the dataset with which you are working. You may still change these in your workflows at any time, but these are good places to start.

Download and Import Sentinel-1 Scenes

This section provides general steps for choosing, downloading, and importing Sentinel-1 data into SARscape.

Choose Sentinel-1 Scenes

Here are some things to consider when choosing Sentinel-1 scenes:

When you search and order Sentinel-1 Level-1 data from the Copernicus Sentinel Open Access Hub or other data portal, you can download Single Look Complex (SLC), Ground Range Detected (GRD), or Ocean (OCN) data. An SLC dataset contain both amplitude and phase, recorded as complex numbers. Both are needed if you will be creating coherence images or doing interferometry. An SLC dataset provides the highest possible spatial resolution.

If you are only interested in amplitude (pixel intensity) and will not be doing interferometry, you can download GRD data as long as the spatial resolution is sufficient for your needs. GRD data is already preprocessed to ground range but still needs to be geocoded. The primary advantage of GRD data is a much smaller compressed file size (approximately 1.5 GB) compared to SLC data (7 to 9 GB). However, GRD data may not be available in the same high resolution as SLC data.

If you will be using multiple scenes for change detection or interferometry, the scenes must be in the same orbital direction (ascending or descending), and from the same relative orbit.

Download Sentinel-1 Scenes

Depending on your internet connection, downloading a full Sentinel-1 Level-1A SLC dataset can take several minutes to several hours.

You do not need to download any data for this tutorial; however, instructions are provided for downloading Sentinel-1 data on your own at a later time. To skip these steps and continue with the interactive part of the tutorial, go to the Open and Display Intensity Images section.

You can search and order Sentinel-1 data from the following sources:

You must register for a free account for these sites if you have not done so already.

Another option is to use the SARscape Sentinel Download tool in the ENVI Toolbox. This is a convenient option, especially for downloading multiple scenes. The following steps describe this process:

  1. In the ENVI Toolbox, select SARscape > Import Data > Sentinel Download. The Sentinel Data Download dialog appears.
  2. Define the geographic location you are interested in. All full Sentinel-1 scenes that intersect the specified geographic extent will be downloaded. This step does not define any spatial subsets for downloading. The options for defining a geographic extent are as follows:
    • Click the Optional Files tab. Here, you can select a shapefile that defines the geographic area you are interested in. All Sentinel-1 scenes that intersect the footprint of the shapefile will be downloaded.

      • Tip: You can create a shapefile in ENVI by creating a new vector layer on top of a raster that is georeferenced to a standard projection. Export the vector to a shapefile on disk.

    • Or, click the Parameters tab and enter geographic coordinates (in decimal degrees) in the WEST, NORTH, EAST, and SOUTH fields.
  3. Click the Parameters tab and enter values for the search criteria, especially the following:
    • Acquisition time (From and To)
    • Orbit direction: Choose Ascending, Descending, or ALL. If you will be using multiple scenes for change detection or interferometry, the scenes must be in the same direction. The ALL option is for dual-pair interferometry (not covered in this tutorial) to resolve both vertical and horizontal displacement. If only horizontal displacement is of interest, then the Ascending or Descending options are sufficient.
    • Product Type: Choose from Single Look Complex, Ground Range, or All.
    • Acquisition Mode: IW (Interferometric Wide) is suitable for most applications.
    • Polarisation Model: Choose from VV+VH, VV, HH+HV, HH, or All.
  4. Under the Parameters tab, enter your Copernicus login credentials in the Login-USERNAME and Login-PASSWORD fields.
  5. Under the Parameters tab, set Unzip Files to True.

    6. The following image shows an example:

  6. Click the Output Files tab.
  7. Choose a directory and filename for the Progress file name. The progress file will contain a running list of all data files that have been fully downloaded. Its purpose is to prevent the same file from being downloaded again. If you use the Sentinel Download tool in the future, you can choose a progress file that you previously created. The tool will not download any files that have been previously downloaded.
  8. In the Unzip files to this directory field, specify a directory where you want to extract the downloaded files.
  9. Click Exec in the Sentinel Data Download dialog. A new command window appears and reports the progress of the download. You can continue to use ENVI and SARscape tools during this time.

When download is complete, the files are automatically unzipped to the working directory that you specified. Using an SLC dataset as an example, the directory containing the data files will be named S1B_IW_SLC_1SV_<acquistion time>_*.SAFE. The directory will contain a manifest.safe file, a PDF report, and the following subdirectories: annotation, measurement, preview, and support.

Import Sentinel-1 Data into SARscape

After downloading Sentinel-1 data, you must import the data into SARscape.

You do not need to import any data for this tutorial; however, instructions are provided for future reference. These steps were used to create the intensity image that you will use later in this tutorial.

  1. From the ENVI Toolbox, select SARscape > Import Data > SAR Spaceborne > Single Sensor > SENTINEL-1. The Import Sentinel-1 dialog appears.
  2. Under the Input Files tab, click Browse under Input File List. A Select Input Files dialog appears.
  3. Navigate to your working directory and select the file manifest.safe. Click Open.
  4. Optional: Click the Optional Files tab and select a shapefile that defines the geographic extent of your area of interest. This can significantly reduce processing time, as only the radar bursts that intersect the shapefile will be imported.
  5. Click the Parameters tab.
  6. Setting the Make power QL option to True will automatically create a multilooked intensity image so that you do not have to perform this step separately at a later time.

    7. Multilooking is a process by which the pixels in an SLC dataset are averaged in the range direction. This is essentially a slant-range to ground-range conversion that averages adjacent oblong pixels and creates a square pixel from them. As an added benefit, the averaging also smooths the image and reduces some speckling effects. See the Multilooking section of the sarmap help for details. You can access the sarmap help by selecting SARscape > Help in the ENVI Toolbox.

    The Make power QL option was set to True to create the intensity image used in this tutorial. If you want more control over the multilooking parameters, set this option to False. Then use the Multilooking tool later under SARscape > Basic > Intensity Processing. You can use the Multilooking tool to set the number of looks used in the range or azimuth direction, as well as the grid size for the suggested number of looks.

  7. Under the Parameters tab, choose a Polarization option. The choices are ALL, Copolarization only (HH or VV), or Crosspolarization only (HV or VH). If you will be doing interferometry, the Crosspolarization only option is recommended in order to reduce processing time, since you should only use cross-polarized data for interferometric analysis.
  8. Under the Parameters tab, setting the Make mosaic same track option to True will automatically mosaic the radar bursts that were acquired sequentially along the same track.
  9. Click the Output Files tab.
  10. Select an output directory and filename for the output files that will be created.
  11. Click the Exec button in the Import Sentinel-1 dialog.

When processing is complete, the output files are written to the location you specified in Step 9. Refer to the Import Data – SAR Spaceborne – SENTINEL-1 topic in the sarmap help for more information about the structure and content of the output files.

Open and Display Intensity Images

In this section, you will explore a Sentinel-1 intensity image that covers a region of Chile in December of 2017. Follow these steps:

  1. From the ENVI main menu bar, select File > Open.
  2. Navigate to the SARGettingStarted directory. You created this directory earlier in the Files Used in This Tutorial section.
  3. Navigate to the 2017-12-12-SLC-Power directory and select the file sentinel1_83_20171212_095750732_IW_SIW1_D_VH_slc_list_pwr. Click Open. An Interferometric Wide (IW) Single Look Complex (SLC) intensity image appears in the ENVI display.
  4. Press the F12 key on your keyboard to view the full extent of the image.

This is a spatial subset of a Sentinel-1 multilooked SLC intensity image. The radar data were acquired from a descending pass, so the image appears flipped. The bottom of the image represents a northeastern direction. Later you will use the Geocoding and Radiometric Calibration tool to georeference the image, which will correct the orientation. The dark region on the right side of the image is the Pacific Ocean. The image covers a portion of Corcovado National Park. The lake in the upper-left corner is Lago Yelcho.

The following steps were taken to create this image:

The pixel values in this image represent the intensity of the backscatter. Intensity is amplitude squared. When SLC datasets are processed with multilooking, the resulting intensity images are called power images, with the characters _pwr appended to the filenames. Intensity images are useful in change detection. When multiple images are coregistered to the same geographic location, they can help answer the question, "Did a pixel get brighter or darker over time?" Intensity images are also used to create coherence images, which are used in SAR processing for flood mapping and landslides.

Intensity images show how different surface types reflect incoming energy back to the sensor. For example, smooth bodies of water appear black. They are flat surfaces that reflect incoming energy away from the sensor—a process known as specular reflection. Bright pixels indicate areas where a large fraction of the incoming energy is reflected back to the sensor. This occurs most often with rough surfaces in a process known as diffuse reflection. Bright pixels can also result from surfaces that are inclined toward the sensor. In urban areas, buildings often appear very bright because incoming energy is bounced off of them multiple times—a process known as double bounce. For more information, consult the references at the end of the tutorial.

The image you are viewing represents cross-polarized intensity (VH). Cross-polarized images are often better than co-polarized images (VV or HH) in applications such as flood detection. VV images are more sensitive to changes in the wind-induced surface roughness of water, which can result in inaccurate change detection over water. To view a co-polarized (VV) image, follow these steps:

  1. Select File > Open from the ENVI main menu bar.
  2. Navigate to the SARGettingStarted directory.
  3. Select the file sentinel1_83_20171212_095750732_IW_SIW1_D_VV_slc_list_pwr and click Open. The VV image displays over the VH image in the ENVI display.
  4. Toggle between the two images by unchecking and checking the VV layer in the Layer Manager:

The following images show the differences in intensity between a cross-polarized (VH) image and co-polarized (VV) image over a large lake. The VV image shows more variation in intensity within the lake.

To get meaningful scientific results from intensity images—particularly when comparing multiple images over time—you must do some further processing with the images. The most critical processing steps include multilooking, coregistration, spatial subsetting, filtering, and geocoding and radiometric calibration. You will explore some of these processes next.

Process Intensity Images

In this section, you will learn how to:

Multilooking is typically the first processing step before sample selection; however, the intensity images used in this tutorial already have already been corrected for multilooking by setting the Make power QL option to True in the Import Sentinel-1 Data tool. Multilooking is the process by which SLC image pixels are averaged in the range and/or azimuth direction, thus converting from slant range resolution to ground range resolution.

Because you are only working with a single image in this tutorial, you will not perform coregistration. You would need to coregister multiple images if you were doing change detection or other time-series analysis. Coregistration is typically done after multilooking.

Create Spatial Subsets (Sample Selection)

In this step, you will create spatial subsets from the VH and VV intensity images. The subsets cover a region around Villa Santa Lucia, Palena Province, Los Lagos Region in Chile. This community was devastated by a landslide that occurred after heavy rains on 16 December 2017. The images in this tutorial were acquired before the landslide, on 12 December.

Defining a spatial subset allows you to focus analysis on a specific area, while reducing processing time and output file sizes.

  1. In the ENVI Toolbox, select SARscape > General Tools > Sample Selections > Sample Selection SAR Geometry Data. This tool is used to subset SLC or intensity (power) data using a shapefile that was drawn on a non-geocoded SAR scene. The shapefile defines the boundary of the spatial subset. You would use the other tool, Sample Selection Geographic Data, if you had a shapefile that was derived from a geocoded scene.
  2. In the Sample Selection SAR Geometry Data dialog, click the Browse button under the Input Files tab.
  3. Navigate to the SARGettingStarted\2017-12-12-SLC-Power directory.
  4. Use Ctrl-click to select the following files, then click Open:

    • sentinel1_83_20171212_095750732_IW_SIW1_D_VH_slc_list_pwr

    • sentinel1_83_20171212_095750732_IW_SIW1_D_VV_slc_list_pwr

  5. Click the Optional Files tab.
  6. Click the File Select button next to Area of Interest.

  7. In the SARGettingStarted directory, select the file StudySite.shp. Click Open. This shapefile defines the spatial subset you will use.

  8. Click the Parameters tab.
  9. Click SELECT next to the Geographical Region field and select the False option. The shapefile was derived from the intensity image, and it is not geocoded.
  10. Click inside the field next to Use Min and Max Coordinates and select the True option. This will clip the spatial subset to a rectangular region if the shapefile itself is not perfectly rectangular.
  11. Click the Output Files tab and notice that the output filenames will be appended with _cut_pwr. They will be saved to the SARGettingStarted directory. You do not need to change anything here.
  12. Click the Exec button in the Sample Selection SAR Geometry Data dialog.
  13. When the Completed dialog appears, click OK. The spatial subsets for the VH and VV images appear in the Layer Manager and the ENVI display.
  14. Click the Close button in the Sample Selection SAR Geometry Data dialog.
  15. Right-click on the following layers in the Layer Manager and select Remove. These are the original intensity images:

    • sentinel1_83_20171212_095750732_IW_SIW1_D_VH_slc_list_pwr

    • sentinel1_83_20171212_095750732_IW_SIW1_D_VV_slc_list_pwr

    Only the _cut_pwr images should be listed.

  16. Press the F12 key on your keyboard to see the full extent of the subsets.

Apply Image Filtering

In this step, you will apply a spatial filter to the subset intensity images to reduce the speckled appearance. You will use a mean filter, which replaces each pixel with the mean value of its surrounding pixels in a 5 x 5 pixel moving window.

  1. In the ENVI Toolbox, select SARscape > Basic > Intensity Processing > Filtering > Single Image Filtering.
  2. In the Single Image Filtering dialog, click Browse under the Input Files tab.
  3. Use Ctrl-click to select both _cut_pwr images that you created in the previous section. Click Open.
  4. Click the Parameters tab.
  5. Click SELECT next to the Filter Method field, then select the Mean option.
  6. Leave the other parameters at their default values.
  7. Select the Output Files tab and notice that the output filenames will be appended with _fil to indicate filtering. They will be saved to the SARGettingStarted directory. You do not need to change anything here.
  8. Click the Exec button in the Single Image Filtering dialog.
  9. When the Complete dialog appears, click OK. The filtered images appear in the Layer Manager and ENVI display. Notice their smoother appearance, compared to the original images.

  10. Click the Close button in the Single Image Filtering dialog.
  11. In the Layer Manager, right-click on the View layer and select Remove All Layers.

Geocode the Images

In this section, you will perform geometric and radiometric calibration of the filtered intensity images. These steps are important if you will be comparing multiple intensity images over time.

Geocoding requires a DEM. You will need to download the DEM data on your own, as we cannot redistribute certain DEM files. Here are some recommended options:

Follow these steps to perform geocoding and radiometric calibration:

  1. In the ENVI Toolbox, select SARscape > Basic > Intensity Processing > Geocoding > Geocoding and Radiometric Calibration.
  2. In the Geocoding and Radiometric Calibration dialog, click Browse under the Input Files tab.
  3. Use Ctrl-click to select both _fil images you created in the Apply Image Filtering section. Click Open.
  4. Click the DEM/Cartographic System tab.
  5. Select a DEM file. Choose one of the following options:
    • To download SRTM-3 Version 4 DEM data, click the Download DEM button . Select the SRTM-3 Version 4 option, then click the OK button . When the DEM Extraction - SRTM3 Version 4 dialog appears, click the DEM/Cartographic System tab. From the State drop-down list, select GEO-GLOBAL. Click the Exec button. SARscape will search for DEM tiles that match the location of the filtered intensity images. It will mosaic the tiles if multiple tiles are found.
    • If you downloaded an ASTER GDEM, click the Open button . In the Select DEM File dialog, navigate to the location where you saved the DEM. Change the File name filter to *.*. Select the _dem_bil file, then click Open.
  6. In the Geocoding and Radiometric Calibration dialog, click the Parameters tab.
  7. Accept all of the default values. (You can optionally change the Output type to dB, if desired.)

  8. Click the Output Files tab, and notice that the output filenames will be appended with _geo. The files will be saved to the SARGettingStarted directory. You do not need to change anything here.
  9. Click the Exec button.
  10. When the Completed dialog appears, click OK. ENVI creates a raster series with the geocoded VH and VV images. It displays the VH image.
  11. Press the F12 key on your keyboard to view the full extent of the geocoded and calibrated VH image.
  12. Click the Close button in the Geocoding and Radiometric Calibration dialog.

    13. The following image shows an example of a geocoded VH image created using an ASTER GDEM.

  13. Right-click in the middle segment of the Status bar and select Raster Data Values. The Status bar is located at the bottom of the ENVI application. It is divided into three segments.
  14. Move the cursor over the image. The "Data" line in the Status bar reports the pixel data values (in units of intensity or decibels); for example:

    15. Also notice that the left segment of the Status bar reports the geographic latitude and longitude coordinates as you move around the image.

    ENVI creates a raster series (also called a time series) of the geocoded VH and VV images. The raster series is indicated by a icon in the Layer Manager. This raster series is not helpful at the moment, as it only contains two images. You will display a different dataset in the following steps.

  15. Right-click the raster series layer in the Layer Manager, and select Remove.
  16. Click the Data Manager button in the ENVI toolbar. The Data Manager lists two separate entries for the geocoded dataset. The first dataset is the raster series as indicated by _geo_db_series in the filename. The second dataset is a metaspectral dataset (also called a band stack) of the geocoded VH and VV images. The filename for the metaspectral dataset is appended with _geo_db_meta. This dataset is highlighted in the following figure:

  17. In the Layer Manager, click the + icon next to the sentinel1_83*_geo_db_meta layer. This expands the layer so that you can tell what image is currently displayed in the view. It shows that the Meta 1 layer (the geocoded VH band) is currently displayed.

  18. In the Data Manager, select the Meta 2 (Band 1...) band, then click the Load Grayscale button. Now the VV image is displayed in the view.
  19. Uncheck and check the VV layer in the Layer Manager to toggle between it and the VH image.

Create a Color Composite

A common task in SAR analysis is to create a color composite image from different polarizations. This can help to visually distinguish between different surface features such as mountains, cities, and water bodies. In this section, you will create a color composite of the geocoded metaspectral dataset using the following polarization combinations:

First, create a band ratio of the VV and VH images:

  1. In the ENVI Toolbox, select Band Algebra > Band Ratios.
  2. In the Band Ratio Input Bands dialog, select the Meta 2 band. The Numerator field is populated with the name of the VV image.
  3. Select the Meta 1 band. The Denominator field is populated with the name of the VH image.

  4. Click the Enter Pair button. The VV/VH ratio is added to the Selected Ratio Pairs section.
  5. Click OK.
  6. In the Band Ratios Parameters dialog, select to output the result to Memory.
  7. Click OK. When processing is complete, the VV/VH ratio image appears in the display.
  8. In the Data Manager, click to expand the Band Selection area. The red box is currently selected.
  9. Select the Meta 2 band. This populates the red box with the geocoded VV band.
  10. Select the Meta 1 band. This populates the green box with the geocoded VH band.
  11. Select the Ratio band. This populates the blue box with the geocoded VV/VH band.

  12. Click the Load Data button. The color composite appears in the display.

    13. The different colors, especially yellow and red, highlight variations in topography.

  13. From the ENVI menu bar, select Views > Reference Map Link. A separate dialog appears with a map view that shows the geographic location of the image (indicated by a cyan-colored box).

  14. Use the Zoom tools in ENVI to zoom in and out of the image. The Reference Map Link dialog updates to show the geographic location of the view extent.
  15. When you are finished viewing the color composite image, click the Close All Files button in the Data Manager.
  16. Close the Data Manager.

This concludes the tutorial.

Using the ENVI Modeler for Batch Processing

So far, you have completed several processing steps using a single image. What if you have multiple input images to process, for example, with change detection or interferometry? An efficient way to batch-process multiple images in ENVI SARscape is to use the ENVI Modeler.

The ENVI Modeler is a visual programming tool that leverages ENVI's powerful analytics wtih a simple user interface. It allows you to create custom workflows using different inputs and parameters. Most SARscape analytics are available to use with the ENVI Modeler.

References

Closson, D., editor. Land Applications of Radar Remote Sensing. IntechOpen (2014), 307 pp.

Committee on Earth Observation Satellites (CEOS). "A Layman’s Interpretation Guide to L-band and C-band Synthetic Aperture Radar Data." Version 2.0 (2018). Available online at http://ceos.org/ard/files/Laymans_SAR_Interpretation_Guide_2.0.pdf.

Davies, R. "Chile – Heavy Rain Causes Deadly Landslide in Los Lagos Region." FloodList.com. http://floodlist.com/america/chile-landslide-los-lagos-region-december-2017, accessed January 2019.

European Space Administration (ESA). "Sentinel-1 SAR User Guide." Available online at https://sentinel.esa.int/web/sentinel/user-guides/sentinel-1-sar.

Jarvis, A., H. Reuter, A. Nelson, and E. Guevara. "Hole-filled Seamless SRTM Data V4." International Centre for Tropical Agriculture (2008). Available online at http://srtm.csi.cgiar.org.

Massonnet, D., and J.-C. Souyris. Imaging with Synthetic Aperture Radar. EPFL Press (2008), 250 pp.

NASA/METI/AIST/Japan Spacesystems, and U.S./Japan ASTER Science Team. ASTER Global Digital Elevation Model (2009). Distributed by NASA EOSDIS Land Processes DAAC, https://doi.org/10.5067/ASTER/ASTGTM.002.