= In-house developed scripts =

This is a list of scripts that have been developed at ARSF-DAN to aid in processing and handling of the data. As these may be useful for further processing of ARSF data descriptions are included here. If you have an interest in using one of these scripts, or would like to know if one would be useful for what you are trying to do, then please [wiki:AboutUs#ContactUs contact us] and we can supply them to you with limited help. 

Please note that these are specifically designed for processing using linux systems as set up at ARSF-DAN. There are no guarantees that they will work with other system set ups. Some scripts are simply just wrappers for using other free packages (such as liblas or LAStools). A lot of these scripts are only suitable for working on raw data and not the standard delivered level-1 data.

=== LiDAR ===

 || '''Name''' || '''Description''' ||
 || check_ascii_lidar(.sh) || Linux bash script that scans ASCII lidar and reports min/max values || 
 || classify_las || Linux bash program for auto-classifying noisy points in LAS files || 
 || get_first_return.sh || Linux bash scan ASCII LiDAR files and returns only first returns || 
 || lag || Linux bash lidar point cloud viewer ||
 || make_lidardem_or_intensity.sh || Linux GRASS script that makes a simple DEM or intensity mosaics from ASCII lidar files  ||

=== Raw hyperspectral data ===

 || '''Name''' || '''Description''' ||
 || bil_binning.py || spectrally bins (x2) a hyperspectral raw file || 
 || cal_radiometric.py || Generates a calibration curve in each band given input data in BIL or BSQ format and a known lamp file || 
 || check_fsm.py || Works out the corrected value for frame shift smear at a given band assuming a constant DN value through the spectrum || 
 || check_qpftiming.py || Test specified Eagle/Hawk framerates against actual framerates calculated from qpfTiming || 
 || checkpeaks.py  || 	Matches measured spectral lines to fityk-detected peaks and eagle/hawk pixel numbers for use in spectral calibration || 
 || dummy_linecount.py || Replaces a broken line counter on the first band of eagle and hawk || 
 || gen_bandsets.py  || Generates bandset (.prn, .bnd, .wls) files from a wavelength scale file || 
 || gen_synth_radcal.py || Generates a synthetic Eagle or Hawk calibration file || 
 || gen_synth_raw.py || Generates a synthetic Eagle or Hawk dataset || 
 || gen_synth_sbet.py || Generates a synthetic SBET file || 
 || generate_prn.py || Generates a .prn file from some subset of bands in a given .wls file || 
 || nav2txt || Output contents of an AISA nav file to an ASCII text file || 
 || split_autodark.py || split a line from it's dark frames || 
 || splitline || split eagle and hawk flightlines || 
 || slice_nav.py || split nav files || 
 || specim_gap_check.py || Searches Eagle/Hawk raw files for dropped frames by looking at the band 1 frame counter || 


=== Camera ===

 || '''Name''' || '''Description''' ||
 || photo2thumb.sh || Uses the Linux convert utility to convert TIFF files to smaller JPEGS ||

=== General ===

 || '''Name''' || '''Description''' ||
 || asterdem.sh  || generates a DEM from ASTER data using GRASS ||
 || nextmapdem.sh  || generates a DEM from nextmapdata using GRASS ||
 || dimfixer.py  || Truncates BIL files so that the file size matches what the header file says it should || 
 || fastQC || QC viewer of BIL data files ||
 || get_sbet_bounds.py || Gets North/South/East/West extent of (part of) an SBET file in lat/lon || 
 || logwriter.py || Outputs mean altitude, heading and speed from an SBET file for a number of Eagle or Hawk lines || 
 || make_mosaic.sh || Script to convert GeoTIFFs into JPGs using GRASS and create a mosaic image || 



=== Python Libraries ===

 || '''Name''' || '''Description''' ||
 || band_reader.py  ||  reads AISA band files || 
 || data_handler.py  ||  BIL/BSQ reading/writing library || 
 || sbet_handler.py  ||  functions to manipulate SBET files and Specim nav files || 
 || sol_reader.py  ||  sol reading library ||