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ISIS Application Documentation


kaguyasp2ascii

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Converts Kaguya SP (Spectral Profiler) file to a tab delimited text file

Overview Parameters

Description

This program will read a binary SELENE Kaguya SP (Spectral Profiler) data file (downloaded as a .spc file from the archive site) and create a user-specified, tab-delimited text file. The multi-column ASCII text file will contain one record for each of the 296 wavelengths (bands or channels) in the SP file. The bands are derived from 3 separate sensors, with wavelengths as follows: UVVIS wavelength = 512.6 -1010.7 nm; NIR1 wavelength = 883.5 - 1676.0 nm; NIR2 wavelength = 702.1-2587.9 nm. Each record in the output file will contain ancillary data and all of the observations for a specific wavelength. You can limit the number of observations that are listed by using the MINOBS and MAXOBS parameters. The ancillary data include a quality assessment (QA) parameter, raw DN, radiance, and ref_1 and ref_2 (reflectance values that have been photometrically corrected using values for highlands and mare, respectively) for each wavelength and each observation. SP binary data files can have less than 10 observations or more than 50. This program works on both Level 2B and Level 2C products from Kaguya, with two caveats: the NIR portions of the Level 2B products are not calibrated or photometrically corrected, but the L2C products have been fully calibrated and photometrically corrected.

The documents in the kaguyasp2ascii/assets directory provide information about the Kaguya Spectral Profiler data. The directory also contains a summary of what the different Quality Assessment values mean (from p. 82 of the LISM SPICE documentation).

Note that this program does not process the SP data in any way once the binary data is converted to ASCII. For example, you likely would not want to work with SP data that have oblique viewing angles or are poorly illuminated (these must be filtered from the archive site), or you may want to remove redundant or erroneous data at the instrument joins (e.g., spikes in DN values at the ends of the VIS, NIR1, NIR2). For the latter, the QA values will help you to identify these. QA values with any of the three left-most bits set to 1 can be removed from each spectrum.

References:
Yamamoto, S. et al. (2011) Preflight and in-flight calibration of the spectral profiler onboard the SELENE (Kaguya). IEEE Trans. Geosci. Remote Sens. 49 (11), p. 4660-4676.
Yamamoto, S. et al. (2014) Calibration of NIR2 of Spectral Profiler onboard Kaguya/SELENE, IEEE Trans. Geosci. Remote Sens. 52 (11), p. 6882-6898.
Yokota, Y., et al. (2011) Lunar photometric properties at wavelengths 0.5-1.6mm acquired by SELENE Spectral Profiler and their dependency on local albedo and latitudinal zones. Icarus, 215, 639-660, http://dx.doi.org/10.1016/j.icarus.2011.07.028.


Categories


History

Janet Barrett2014-02-19 Original version. This program imports binary data from a Kaguya Spectral Profiler file and puts the data into a tab delimited table.
Kristin Berry2015-08-24 Updated to deal with format change for newer files . Now will output both reflectances and calibrated NIR2 data if available. Also, updated to put actual QA information in the output file, which was not happening correctly before, and updated online documentation to match Lisa Gaddis's rewrite. Additionally, headers are now tab-separated, rather than comma-separated. Fixes #2218
Kristin Berry2015-09-18 Backward Compatibility Issue: The application name was changed from kaguyasp2isis to kaguyasp2ascii since this application does not output an ISIS Cube, which could impact processing scripts/pipelines which use the old application name.

Parameter Groups

Files

Name Description
FROM Input Kaguya SP file
TO Output Kaguya text file

Limit Parameters

Name Description
MINOBSMinimum observation
MAXOBSMaximum observation
X

Files: FROM


Description

This is the input Kaguya SP file. For an attached label, use the .spc file, or for a detached label, use the .lbl file.

Type filename
File Mode input
Filter *.lbl *.spc
Close Window
X

Files: TO


Description

The output file will be formatted as a tab delimited file and will contain all requested observations for a single wavelength in each record of the file. Each observation will include the raw, radiance, reflectance, and QA information. If two reflectances are available, as in newer-format files, both will be included in the output file.

Type filename
File Mode output
Close Window
X

Limit Parameters: MINOBS


Description

This is the minimum observation of the observation range for which information will be obtained from the input file. If no value is specified, then the minimum will be set to 1.

Type string
Default None
Close Window
X

Limit Parameters: MAXOBS


Description

This is the maximum observation of the observation range for which information will be obtained from the input file. If no value is specified, then the maximum will be set to the maximum observation in the input file.

Type string
Default None
Close Window