ISIS Application Documentation
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Import NEAR MSI files into ISIS format
Overview | Parameters | Example 1 |
Description
This program will import raw images, acquired from the Near Earth Asteroid
Rendezvous - Shoemaker (NEAR Shoemaker) mission's Multispectral Imager
(MSI) instrument, to ISIS data file format.
The raw image must be in FITS (Flexible Image Transport) format and
have a PDS label file that points to the location of the FITS image. You
must input either the label file or the FITS file for the "TO" input
parameter. Projected images are not supported. Please note if the FITS
file is given, the label file must exist in the same directory or the
program will throw an error.
This program will verify that the input files are valid by checking the
following label keyword values. An error will be thrown if any of these
criteria are not met.
Image TrimmingShortly after orbit insertion around Eros, the NEAR spacecraft experienced a failed burn that contaminated the MSI instrument with hydrazine. The NEAR/MSI team developed a preliminary remediation [1] of the blur effect of the contamination using FFTs to correct the point spread function (PSF). A residual side effect of this correction was degradation of ~33 pixels on all edges of the images. As a result, by default, NEAR/MSI images are trimmed 33 pixels around all edges after import. MSI images requiring trmming of these data are of the form m0132069107f4_2p_iof_dbl.img.
Additional remediation work of the PSF function used to correct MSI
images was performed by Golish [2] that resulted in an enhanced PDF
correction that did not introduce edge-artifacts as was seen in [1].
The TRIM parameter was added to optionally retain the 33 pixels around
the image edges when the dataset from [2] is used. File names that do
not require trimming are of the form m0132069107f4_2p_iof_gbl.img (note
the Note the images produced by Golish [2] have already been expanded. So msi2isis was altered to check for the expanded size (in lines only) to allow for the full frame to be ingested. In this case, the intermediate step to interpolate in the line dimension to expand the the number of lines from 244 to 412 is not needed and excluded from ingestion processing. All other (label) checks were left to complete the validation of the input files. References1. Li, H., et al. (2002) Preliminary Remediation of Scattered Light in NEAR MSI Images. Icarus 155, 244-252. https://doi.org/10.1006/icar.2001.6745 2. Golish, D.R., et al. (2021) Improved Remediation of NEAR MSI Images of Asteroid (433) Eros. LPSC LII, Abstract #1682. CategoriesRelated Objects and DocumentsApplicationsHistory
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U.S. Department of the Interior | U.S. Geological Survey ISIS | Privacy & Disclaimers | Astrogeology Research Program To contact us, please post comments and questions on the USGS Astrogeology Discussion Board To report a bug, or suggest a feature go to: ISIS Github File Modified: 02/21/2025 19:28:13 |
Parameter GroupsFiles
Scaling Parameters
Trimming Parameters
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U.S. Department of the Interior | U.S. Geological Survey ISIS | Privacy & Disclaimers | Astrogeology Research Program To contact us, please post comments and questions on the USGS Astrogeology Discussion Board To report a bug, or suggest a feature go to: ISIS Github File Modified: 02/21/2025 19:28:13 |
Name of the input NEAR MSI image file to be imported into ISIS format. You may enter the label or the image file. If the image file is given, the program will search in the same directory for a label file with the same base name as the image file base name.
Type | filename |
---|---|
File Mode | input |
Filter | *.lbl *.fit *.fits |
Name of the ISIS output cube file that has been imported, enlarged, flipped, and trimmed.
Type | cube |
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File Mode | output |
Filter | *.cub |
This is the type of interpolation to be performed on the input when the image is enlarged from 537 samples x 244 lines to 537 samples x 412 lines.
Type | string | ||||||||||||
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Default | CUBICCONVOLUTION | ||||||||||||
Option List: |
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This parameter is provided to turn off trimming 33 pixels from the edge of images. When TRIM=TRUE, 33 pixels on all sides of the expanded image are set to NULL but not removed. The source of this degradation is image edge-effects created from the remediation of hydrazine contamination of the MSI filters. If TRIM=FALSE, no pixels around the edge of the images are NULLed. This is useful to retain image edges that originate from several alternative archive sources [2].
Type | boolean |
---|---|
Default | true |
U.S. Department of the Interior | U.S. Geological Survey ISIS | Privacy & Disclaimers | Astrogeology Research Program To contact us, please post comments and questions on the USGS Astrogeology Discussion Board To report a bug, or suggest a feature go to: ISIS Github File Modified: 02/21/2025 19:28:13 |