ISIS Application Documentation
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Combines HiRISE image data with all pixel data in the blobs
This program will create a new image with the calibration pixel data at the top, followed by the main image data. Both the calibration and main image will have the buffer pixels added to the left side and the dark pixels to the right side.
The pixel values are retrieved from either the Isis tables or the main image. The calibration buffer and dark pixels are pulled from the "HiRISE Ancillary" table. The main calibration image pixels come from the "HiRISE Calibration Image" table. The image buffer and dark pixels come from the "HiRISE Ancillary" table. The observation pixels come from the main Isis cube.
The calibration image and observation image pixels of a HiRISE image can be flipped from left to right using the "FLIP" parameter. See the "FLIP" parameter description for details.
The HiRISE cube containing the image and tables from the EDR product. This must be an Isis cube (i.e., "hi2isis" must be run before "higlob").
The output cube containing the main image data, calibration data, buffer pixels and dark pixels.
This is typically channel 1 (discovered after launch!) rather than 0, but this option allows you to choose the channel you want to flip. The default (1) is the one designated as the channel to flip to best assist in calibration analysis.
If FLIP matches the value of the ChannelNumber keyword in the Instrument group, then both the observation and calibration image data will be filpped left to right. This does not modify the byte order of the individual pixels, and does not flip any of the buffer or dark pixels.
To ensure that you flip no channel, set FLIP to "None".