For the complete documentation index, see llms.txt. This page is also available as Markdown.

Arguments

input_path

Path to image files taken from supported sensors. Choose the session folder of your images. This will cause the script to correct the images in each subfolders for all 5 multispectral band and ignore the rgb folder.

--calibration_id "CALIBRATION_ID", -c CALIBRATION_ID

Identifier in the name of the image that denotes it is from the calibration set. If not specified, defaults to "CAL".

--output_path OUTPUT_PATH, -o OUTPUT_PATH

Path to output folder at which the corrected images will be stored. If not supplied, corrected images will be placed into the input directory.

--no_ils_correct, -i

If selected, Incident Light Sensor correction will not be applied to the images.

--no_reflectance_correct, -r

If selected, reflectance correction will not be applied to the images.

--delete_original, -d

Overwrite original 12-bit images with the corrected versions. If selected, corrected images are renamed to their original names. If not, an extension is added.

--exiftool_path EXIFTOOL_PATH, -e EXIFTOOL_PATH

Path to ExifTool executable. ExifTool is required for the conversion; if not passed, the script will use a bundled ExifTool executable.

--uint16_output, -u

If selected, scale of output values will be adjusted to 0-65535 and dtype will be changed to uint16.

Arugment Usage

The correction is done in 3 steps:

  1. Autoexposure correction.

  2. Incident Light Sensor correction.

  3. Reflectance correction.

Autoexposure Correction

Sensors simulate longer exposures and wider apertures for subjects with lower upwelling radiance. These scripts correct by dividing pixel values by EXIF ISOSpeedRatings * EXIF ExposureTime

Incident Light Sensor (ILS) Correction

Downwelling radiance may change over the course of a flight as clouds pass overhead. These scripts correct by dividing pixel values by a rolling average of Incident Light Sensor readings (Camera:SunSensor) on images taken within 3 seconds of the corrected image. Correcting for ILS will standardize the DN (digital number) of your images based on the differences in incident light.

Reflectance Correction

Sensors measure upwelling radiance, not reflectance. Radiance is dependent on unpredictable environmental conditions, and without a reference point with known reflectance, it is impossible to calculate. By beginning a flight with a photo of a panel with known reflectance, that panel's upwelling radiance can be used to standardize measurements.

These scripts correct by multiplying pixel values by slope coefficient (calculated based on known calibration panel reflectance values).

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