[doris] 03/05: Add more man pages
Antonio Valentino
a_valentino-guest at moszumanska.debian.org
Wed Sep 13 21:57:09 UTC 2017
This is an automated email from the git hooks/post-receive script.
a_valentino-guest pushed a commit to branch master
in repository doris.
commit b51757d4065fd2b68eeabf317f1da5882fa18c60
Author: Antonio Valentino <antonio.valentino at tiscali.it>
Date: Wed Sep 13 20:46:39 2017 +0000
Add more man pages
---
debian/TODO | 32 +++-
debian/changelog | 3 +
debian/man/ascii2ascii_UTM.1 | 72 ++++++++
debian/man/ascii2grdAutoMinMaxHDR.1 | 52 ++++++
debian/man/ascii2ps.1 | 144 ++++++++++++++++
debian/man/baseline.doris.sh.1 | 68 ++++++++
debian/man/coregpm.doris.1 | 115 +++++++++++++
debian/man/cpx2ps.1 | 308 ++++++++++++++++++++++++++++++++++
debian/{ => man}/doris.1 | 0
debian/man/doris.adddummystep.sh.1 | 106 ++++++++++++
debian/man/doris.rmstep.sh.1 | 106 ++++++++++++
debian/man/doris.slant2h4master.sh.1 | 21 +++
debian/man/gammaReadfiles.csh.1 | 37 ++++
debian/man/getorb_rs2.py.1 | 25 +++
debian/man/heightamb.1 | 83 +++++++++
debian/man/lonlatCoh2ascii.1 | 120 +++++++++++++
debian/man/lonlathei2ascii.1 | 120 +++++++++++++
debian/man/phasefilt.doris.1 | 135 +++++++++++++++
debian/{ => man}/plotcpm.1 | 0
debian/man/plotcpm.erroffsets.1 | 92 ++++++++++
debian/{ => man}/plotoffsets.1 | 0
debian/man/rs2_dump_data.py.1 | 78 +++++++++
debian/man/rs2_dump_header2doris.py.1 | 40 +++++
debian/{ => man}/rundoris.1 | 0
debian/man/tsx_dump_data.py.1 | 63 +++++++
debian/man/tsx_dump_header2doris.py.1 | 27 +++
debian/man/viewanddel.1 | 23 +++
debian/manpages | 30 +++-
28 files changed, 1895 insertions(+), 5 deletions(-)
diff --git a/debian/TODO b/debian/TODO
index 72cc97d..e98dd3c 100644
--- a/debian/TODO
+++ b/debian/TODO
@@ -5,6 +5,36 @@ Debian maintainers TODO list
E: doris: needlessly-depends-on-awk depends
-* man pages for all tools
+* man pages for all tools.
+ In principle all tool in the bin directory shall have a manpage.
+ It would be nice that at least the following ones would have a man page:
+
+ - ascii2ascii_UTM
+ - ascii2grdAutoMinMaxHDR
+ - ascii2ps
+ - baseline.doris.sh
+ - coregpm.doris
+ - cpx2ps
+ - csk_dump_data.py
+ - csk_dump_header2doris.py
+ - doris.adddummystep.sh
+ - doris.rmstep.sh
+ - doris.slant2h4master.sh
+ - gammaReadfiles.csh
+ - getorb_rs2.py
+ - heightamb
+ - lonlatCoh2ascii
+ - lonlathei2ascii
+ - phasefilt.doris
+ - plotcpm.erroffsets
+ - rs2_dump_data.py
+ - rs2_dump_header2doris.py
+ - sec2hhmmss.py
+ - tsx_dump_data.py
+ - tsx_dump_header2doris.py
+ - viewanddel
+
+ Some of them have been generated automatically using the help2man utility
+ program but surely need to be improved.
-- Antonio Valentino <antonio.valentino at tiscali.it> Tue, 18 Jan 2011 13:11:13 +0100
diff --git a/debian/changelog b/debian/changelog
index dcc6286..ded9505 100644
--- a/debian/changelog
+++ b/debian/changelog
@@ -12,6 +12,9 @@ doris (5.0.3~beta+dfsg-2) UNRELEASED; urgency=medium
- (build-)depend in tcsh instead of csh
- reformatted with cme
* Added a note in README.debian about why the package is in contrib
+ * Updated debian/TODO
+ * Added man pages for several scripts (pages are now in the
+ dedicated debian/man directory)
-- Antonio Valentino <antonio.valentino at tiscali.it> Sat, 09 Sep 2017 12:43:48 +0200
diff --git a/debian/man/ascii2ascii_UTM.1 b/debian/man/ascii2ascii_UTM.1
new file mode 100644
index 0000000..17df169
--- /dev/null
+++ b/debian/man/ascii2ascii_UTM.1
@@ -0,0 +1,72 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH ASCII2ASCII_UTM "1" "September 2017" "ascii2ascii_UTM v1.0 Doris software, bert kampes, (c)1999-2003" "User Commands"
+.SH NAME
+ascii2ascii_UTM \- transforms (lat,lon,h) files into UTM coordinates
+.SH DESCRIPTION
+ascii2ascii_UTM v1.0 Doris software, bert kampes, (c)1999\-2003
+.IP
+USAGE:
+.TP
+ascii2ascii_UTM
+ascii3column +zone=utmzone
+.TP
+This program transforms the WGS84 "longitude
+latitude height" 3 column
+.IP
+ascii file of Doris (created with philamh2ascii) to UTM coordinates
+using proj. (longitude=lambda, latitude=phi)
+First use program lonlathei2ascii to create the 3 column ascii input file.
+.IP
+THe UTM zone needs to be specified as in the example.
+Alternatively, one could specify +lon_0=\-114 for example (see proj manual).
+.TP
+This script can serve as an example.
+If you want to have another projection,
+.IP
+see the manual of proj and cs2cs how to do this.
+.IP
+EXAMPLE:
+.TP
+ascii2ascii_UTM lonlathei.dat +utm_zone=33
+xyz_utm.dat
+.IP
+See also: http://www.remotesensing.org/proj
+.IP
+USAGE:
+.TP
+ascii2ascii_UTM
+ascii3column +zone=utmzone
+.TP
+This program transforms the WGS84 "longitude
+latitude height" 3 column
+.IP
+ascii file of Doris (created with philamh2ascii) to UTM coordinates
+using proj. (longitude=lambda, latitude=phi)
+First use program lonlathei2ascii to create the 3 column ascii input file.
+.IP
+THe UTM zone needs to be specified as in the example.
+Alternatively, one could specify +lon_0=\-114 for example (see proj manual).
+.TP
+This script can serve as an example.
+If you want to have another projection,
+.IP
+see the manual of proj and cs2cs how to do this.
+.IP
+EXAMPLE:
+.TP
+ascii2ascii_UTM lonlathei.dat +utm_zone=33
+xyz_utm.dat
+.IP
+See also: http://www.remotesensing.org/proj
+.SH "SEE ALSO"
+The full documentation for
+.B ascii2ascii_UTM
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B ascii2ascii_UTM
+programs are properly installed at your site, the command
+.IP
+.B info ascii2ascii_UTM
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/ascii2grdAutoMinMaxHDR.1 b/debian/man/ascii2grdAutoMinMaxHDR.1
new file mode 100644
index 0000000..fd309bd
--- /dev/null
+++ b/debian/man/ascii2grdAutoMinMaxHDR.1
@@ -0,0 +1,52 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH ASCII2GRDAUTOMINMAXHDR "1" "September 2017" "ascii2grdAutoMinMaxHDR v1.0 doris script utilities, nicolas doreye, (c)2006" "User Commands"
+.SH NAME
+ascii2grdAutoMinMaxHDR \- transforms the 3 column ascii file to GMT grd file
+.SH DESCRIPTION
+ascii2grdAutoMinMaxHDR v1.0 doris script utilities, nicolas doreye, (c)2006
+.IP
+USAGE:
+.TP
+ascii2grdAutoMinMaxHDR
+ascii3column
+.IP
+This program transforms the 3 column ascii file of Doris
+(created with LonLat???2ascii) to GMT grd file then remove the header
+in order to be opened by ENVI for instance, then create the appropriate header
+.IP
+First run the program lonlat???2ascii to create the 3 column ascii input file
+.IP
+EXAMPLE:
+.IP
+ascii2grdAutoMinMaxHDR lonlatSomething.dat
+.IP
+See also: http://www.remotesensing.org/proj
+.IP
+USAGE:
+.TP
+ascii2grdAutoMinMaxHDR
+ascii3column
+.IP
+This program transforms the 3 column ascii file of Doris
+(created with LonLat???2ascii) to GMT grd file then remove the header
+in order to be opened by ENVI for instance, then create the appropriate header
+.IP
+First run the program lonlat???2ascii to create the 3 column ascii input file
+.IP
+EXAMPLE:
+.IP
+ascii2grdAutoMinMaxHDR lonlatSomething.dat
+.IP
+See also: http://www.remotesensing.org/proj
+.SH "SEE ALSO"
+The full documentation for
+.B ascii2grdAutoMinMaxHDR
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B ascii2grdAutoMinMaxHDR
+programs are properly installed at your site, the command
+.IP
+.B info ascii2grdAutoMinMaxHDR
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/ascii2ps.1 b/debian/man/ascii2ps.1
new file mode 100644
index 0000000..f6331b5
--- /dev/null
+++ b/debian/man/ascii2ps.1
@@ -0,0 +1,144 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH ASCII2PS "1" "September 2017" "ascii2ps v1.1 Doris software, TUDELFT, (c)1999-2009" "User Commands"
+.SH NAME
+ascii2ps \- create a postscript file of the data in the 3 column ASCII input file
+.SH DESCRIPTION
+ascii2ps v1.1 Doris software, TUDELFT, (c)1999\-2009
+.IP
+USAGE:
+.TP
+ascii2ps
+3col_asciifile
+.IP
+Create a postscript file of the data in the 3 column ASCII input file
+containing "lon lat hei" triplets (output of lonlathei2ascii
+program). GMT is used to interpolate these irregularly distributed
+data to a grid.
+.IP
+This script is intended to be transparent and understandable.
+Please adapt this script to your own needs. (lambda=longitude).
+For example, here one could easily set the correct approximate
+height of the terrain.
+.IP
+The output is a postscript file named "temp.ps".
+.IP
+The steps foreseen to be taken are:
+.IP
+[before running this, create a three column ascii file with lon lat hei
+.IP
+using philamh2ascii program.
+AND optionally convert this 3 column file to UTM coordinates
+using ascii2ascii_UTM
+.IP
+]
+2) Call GMT program xyz2grd to perform interpolation of this data.
+.IP
+the number of points in the output grid is 300.
+.IP
+3) call GMT program cpt to create a color table
+4) call GMT program to create a postscript file
+5) call ghostview to view output.
+.TP
+This script can serve as an example.
+If you want to have another resolution
+.IP
+output grid, for example exactly 100x100 meters, then you will have
+to change this script.
+With the public domain software PROJ.4, you can easily convert the
+WGS coordinates (Doris output) to X,Y values, and then use this script.
+See the script ascii2ascii_UTM for an example how to do this for WGS
+to UTM coordinates conversion.
+.IP
+DEPENDENCIES:
+.IP
+GMT tools (gmtset, minmax, xyz2grd, grd2cpt, psbasemap
+.IP
+psscale, grdgradient, psmask, grdimage, pscoast)
+.IP
+standard UNIX (echo, csh, rm, etc.)
+ghostview
+.IP
+EXAMPLE:
+.IP
+ascii2ps lonlathei.dat
+.IP
+ascii2ps xyz_UTM.dat
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, http://gmt.soest.hawaii.edu/
+.IP
+USAGE:
+.TP
+ascii2ps
+3col_asciifile
+.IP
+Create a postscript file of the data in the 3 column ASCII input file
+containing "lon lat hei" triplets (output of lonlathei2ascii
+program). GMT is used to interpolate these irregularly distributed
+data to a grid.
+.IP
+This script is intended to be transparent and understandable.
+Please adapt this script to your own needs. (lambda=longitude).
+For example, here one could easily set the correct approximate
+height of the terrain.
+.IP
+The output is a postscript file named "temp.ps".
+.IP
+The steps foreseen to be taken are:
+.IP
+[before running this, create a three column ascii file with lon lat hei
+.IP
+using philamh2ascii program.
+AND optionally convert this 3 column file to UTM coordinates
+using ascii2ascii_UTM
+.IP
+]
+2) Call GMT program xyz2grd to perform interpolation of this data.
+.IP
+the number of points in the output grid is 300.
+.IP
+3) call GMT program cpt to create a color table
+4) call GMT program to create a postscript file
+5) call ghostview to view output.
+.TP
+This script can serve as an example.
+If you want to have another resolution
+.IP
+output grid, for example exactly 100x100 meters, then you will have
+to change this script.
+With the public domain software PROJ.4, you can easily convert the
+WGS coordinates (Doris output) to X,Y values, and then use this script.
+See the script ascii2ascii_UTM for an example how to do this for WGS
+to UTM coordinates conversion.
+.IP
+DEPENDENCIES:
+.IP
+GMT tools (gmtset, minmax, xyz2grd, grd2cpt, psbasemap
+.IP
+psscale, grdgradient, psmask, grdimage, pscoast)
+.IP
+standard UNIX (echo, csh, rm, etc.)
+ghostview
+.IP
+EXAMPLE:
+.IP
+ascii2ps lonlathei.dat
+.IP
+ascii2ps xyz_UTM.dat
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, http://gmt.soest.hawaii.edu/
+.SH "SEE ALSO"
+The full documentation for
+.B ascii2ps
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B ascii2ps
+programs are properly installed at your site, the command
+.IP
+.B info ascii2ps
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/baseline.doris.sh.1 b/debian/man/baseline.doris.sh.1
new file mode 100644
index 0000000..33dd70f
--- /dev/null
+++ b/debian/man/baseline.doris.sh.1
@@ -0,0 +1,68 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH BASELINE.DORIS.SH "1" "September 2017" "baseline.doris.sh PROGRAM: baseline.doris.sh -- Obtain baseline parameterization from orbits." "User Commands"
+.SH NAME
+baseline.doris.sh \- manual page for baseline.doris.sh PROGRAM: baseline.doris.sh -- Obtain baseline parameterization from orbits.
+.SH DESCRIPTION
+.TP
+PROGRAM:
+baseline.doris.sh \fB\-\-\fR Obtain baseline parameterization from orbits.
+.PP
+
+.IP
+SYNOPSIS:
+.TP
+baseline.doris.sh
+master.res slave.res
+.IP
+OPTIONS:
+.TP
+master.res
+master result file from doris, precise orbits.
+.TP
+slave.res
+slave result file from doris, precise orbits.
+.IP
+Basically a dummy run is performed, only to get DUMPBASELINE.
+Then from the standard output the appropriate sections are written.
+The DUMPBASELINE card is used, computing the baseline at a grid 15x10,
+then fitting a polynomial through these values (Bperp, theta and range).
+.IP
+EXAMPLE:
+.IP
+baseline.doris.sh master.res slave.res
+.PP
+
+.IP
+SYNOPSIS:
+.TP
+baseline.doris.sh
+master.res slave.res
+.IP
+OPTIONS:
+.TP
+master.res
+master result file from doris, precise orbits.
+.TP
+slave.res
+slave result file from doris, precise orbits.
+.IP
+Basically a dummy run is performed, only to get DUMPBASELINE.
+Then from the standard output the appropriate sections are written.
+The DUMPBASELINE card is used, computing the baseline at a grid 15x10,
+then fitting a polynomial through these values (Bperp, theta and range).
+.IP
+EXAMPLE:
+.IP
+baseline.doris.sh master.res slave.res
+.SH "SEE ALSO"
+The full documentation for
+.B baseline.doris.sh
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B baseline.doris.sh
+programs are properly installed at your site, the command
+.IP
+.B info baseline.doris.sh
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/coregpm.doris.1 b/debian/man/coregpm.doris.1
new file mode 100644
index 0000000..6f0b119
--- /dev/null
+++ b/debian/man/coregpm.doris.1
@@ -0,0 +1,115 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH COREGPM.DORIS "1" "September 2017" "coregpm.doris v1.0, FMR software, Rens Swart (c)2001" "User Commands"
+.SH NAME
+coregpm.doris \- perform step COREGPM iteratively from prompt.
+.SH DESCRIPTION
+coregpm.doris v1.0, FMR software, Rens Swart (c)2001\en
+.IP
+Fit model through the coregistration vectors estimated by FINE;
+.IP
+(ii) Select the vector with largest w\-test and ask user whether it
+.IP
+should be removed.
+If so, remove it, and re\-run Doris (goto (i)).
+If not, stop.
+.IP
+The advantage of this script is that normally the result file needed
+to be edited after each iteration to fit the model.
+Note that the inputfile of Doris should contain cards for
+the resultfiles, run step coregpm, screen info, etc.
+.IP
+SYNOPSIS:
+.IP
+coregpm.doris [\-V] Doris_inputfile
+.IP
+OPTIONS:
+.TP
+\fB\-V\fR
+Verbose flag, default redirect stdout to file: ".doris.stdout.20:25"
+.TP
+input
+Doris input file for step coregpm, if you use run, it is
+like Inputfiles/input.resample
+.IP
+EXAMPLE:
+.IP
+To run Doris without messages to the screen, assuming you
+have a input file named input.cpm, use the following command:
+.IP
+coregpm.doris input.cpm
+.IP
+BUGS:
+.IP
+\- Doris input keywords must be in capitals.
+\- Assume section Start_comp_coregpm is not in result file.
+\- Assume plotcpm is not ran from within Doris (CPM_PLOT OFF).
+\- coregpm.doris output interferes with plotcpm output on screen (if CPM_PLOT ON) (?).
+.IP
+SEE ALSO:
+.IP
+\- http://www.geo.tudelft.nl/doris/ (online user's manual)
+\- phasefilt.fast
+\- helpdoris
+\- run
+.IP
+PROGRAM: coregpm.doris \fB\-\-\fR Perform step COREGPM iteratively from prompt.
+.TP
+(i)
+Fit model through the coregistration vectors estimated by FINE;
+.IP
+(ii) Select the vector with largest w\-test and ask user whether it
+.IP
+should be removed.
+If so, remove it, and re\-run Doris (goto (i)).
+If not, stop.
+.IP
+The advantage of this script is that normally the result file needed
+to be edited after each iteration to fit the model.
+Note that the inputfile of Doris should contain cards for
+the resultfiles, run step coregpm, screen info, etc.
+.IP
+SYNOPSIS:
+.IP
+coregpm.doris [\-V] Doris_inputfile
+.IP
+OPTIONS:
+.TP
+\fB\-V\fR
+Verbose flag, default redirect stdout to file: ".doris.stdout.20:25"
+.TP
+input
+Doris input file for step coregpm, if you use run, it is
+like Inputfiles/input.resample
+.IP
+EXAMPLE:
+.IP
+To run Doris without messages to the screen, assuming you
+have a input file named input.cpm, use the following command:
+.IP
+coregpm.doris input.cpm
+.IP
+BUGS:
+.IP
+\- Doris input keywords must be in capitals.
+\- Assume section Start_comp_coregpm is not in result file.
+\- Assume plotcpm is not ran from within Doris (CPM_PLOT OFF).
+\- coregpm.doris output interferes with plotcpm output on screen (if CPM_PLOT ON) (?).
+.IP
+SEE ALSO:
+.IP
+\- http://www.geo.tudelft.nl/doris/ (online user's manual)
+\- phasefilt.fast
+\- helpdoris
+\- run
+.SH "SEE ALSO"
+The full documentation for
+.B [3J[H[2Jcoregpm.doris
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B [3J[H[2Jcoregpm.doris
+programs are properly installed at your site, the command
+.IP
+.B info [3J[H[2Jcoregpm.doris
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/cpx2ps.1 b/debian/man/cpx2ps.1
new file mode 100644
index 0000000..1b0619b
--- /dev/null
+++ b/debian/man/cpx2ps.1
@@ -0,0 +1,308 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH CPX2PS "1" "September 2017" "cpx2ps v2.1, FMR software, Bert Kampes, (c)1999-2000 \n" "User Commands"
+.SH NAME
+cpx2ps \- Produce various eps codes from complex data files.
+.SH DESCRIPTION
+cpx2ps v2.1, FMR software, Bert Kampes, (c)1999\-2000 \en
+.HP
++++ WARNING: infile missing
+.IP
+SYNOPSIS:
+.IP
+cpx2ps \fB\-w\fR width [\-f format==cr4] [\-q out==mag] [\-e exp==1.0] [\-s sc==1.0]
+.IP
+[\-l 1] [\-L alllines] [\-p 1] [\-P width] [\-M1/1 | \fB\-F1\fR/1]
+[\-m mirror] [\-T title] [\-c cptname==gray] [\-z size==16]
+[\-o epsfile] [\-G grdfile] [\-C cptfile]
+[\-gKSUVZ] [\-h elp] [\-\-] cpxfile
+.IP
+cpxfiddle options:
+.TP
+\fB\-w\fR width
+of complexfile in complex pixels
+.TP
+\fB\-f\fR format
+of complex input file.
+ci2|cr4|cr8 (cr4 is default)
+r4 now also possible, though it limites other options.
+do not use subsampling, mirroring etc, file is cat\-ed.
+.TP
+\fB\-q\fR output
+what is to be computed
+mag|phase|real|imag|normal (mag is default)
+.TP
+\fB\-e\fR exp
+compute scale*output^exp
+.TP
+\fB\-s\fR scale
+compute scale*output^exp
+.TP
+\fB\-l\fR firstline
+cut out complexfile from firstline
+.TP
+\fB\-L\fR lastline
+cut out complexfile up to lastline
+.HP
+\fB\-p\fR firstpixel cut out complexfile from firstpixel
+.TP
+\fB\-P\fR lastpixel
+cut out complexfile up to lastpixel
+.TP
+\fB\-m\fR X Y XY
+mirror option.
+.TP
+\fB\-M\fR 1/1
+multilook factor in X/Y direction
+.TP
+\fB\-F\fR 1/1
+subsample Factor in X/Y direction
+.IP
+GMT options:
+.TP
+\fB\-T\fR title
+title to plot (one word only for now)
+default no title
+.TP
+\fB\-c\fR colortable name of color table (see grd2cpt)
+if \fB\-q\fR mag then gray table is default
+if \fB\-q\fR other then gray table is default
+.TP
+\fB\-S\fR
+add a scale bar (psscale)
+.TP
+\fB\-Z\fR
+continuous color table (grd2cpt)
+.TP
+\fB\-K\fR
+Leave postscript file open after last call to GMT
+.TP
+\fB\-z\fR cm
+largest size of paper
+.TP
+\fB\-U\fR
+Place UNIX time stamp and filename in output
+.IP
+General options:
+.TP
+\fB\-g\fR
+Do not call gv to view result.
+.TP
+\fB\-o\fR
+output postscript file, default=23812.eps (pid)
+.TP
+\fB\-G\fR
+output grd file, default=23812.eps (pid)
+If specified, file is not removed at end
+If file exists, prompted for reuse.
+.TP
+\fB\-C\fR
+output cpt file, default=23812.cpt (pid)
+If specified, file is not removed at end
+If file exists, prompted for reuse.
+.TP
+\fB\-V\fR erbose
+give verbose information
+.TP
+\fB\-h\fR elp
+this help
+.TP
+complexfile
+inputfile, major row order pixel interleaved
+.IP
+EXAMPLES:
+.IP
+Generate a postscript file with phase of complex interferogram
+in file cpxint.raw (complex 2x4B floats) that has 998 range pixels:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qphase\fR \fB\-fcr4\fR \fB\-\-\fR cpxint.raw
+.IP
+The same but with a scale bar, timestamp, and no title:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qphase\fR \fB\-fcr4\fR \fB\-Tnone\fR \fB\-U\fR \fB\-S\fR \fB\-\-\fR cpxint.raw
+.IP
+To plot the magnitude to the power 0.3 of a file in the format
+complex short integers (2x2B) use:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qmag\fR \fB\-fci2\fR \fB\-e0\fR.3 \fB\-\-\fR cpxint.raw
+.IP
+To see a large file it is convenient to set a large size (\fB\-z\fR).
+This file cannot be printed, but viewing it with gv is nice:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qphase\fR \fB\-z200\fR \fB\-\-\fR cpxint.raw
+.IP
+To plot the phase of a hgt file, first create a tmp file with
+the program hgt2file (hgtfile infile linelength tmpfile [ampflag])
+Next, run cpx2ps with appropriate flags for a float file, e.g.
+(Note that this limits some options in scaling etc.):
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-crainbow\fR \fB\-fr4\fR \fB\-\-\fR tmpfile
+.IP
+BUGS:
+.IP
+When mirroring and multilooking/subsampling sometimes
+the number of lines/pixels of the output is computed
+incorrectly. Simply don't use multilooking/subsampling...
+.IP
+Please mail bugs/comments to kampes at geo.tudelft.nl
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, GMT
+.HP
++++ WARNING: infile missing
+.IP
+PROGRAM: cpx2ps \fB\-\-\fR Produce various eps codes from complex data files.
+.IP
+SYNOPSIS:
+.IP
+cpx2ps \fB\-w\fR width [\-f format==cr4] [\-q out==mag] [\-e exp==1.0] [\-s sc==1.0]
+.IP
+[\-l 1] [\-L alllines] [\-p 1] [\-P width] [\-M1/1 | \fB\-F1\fR/1]
+[\-m mirror] [\-T title] [\-c cptname==gray] [\-z size==16]
+[\-o epsfile] [\-G grdfile] [\-C cptfile]
+[\-gKSUVZ] [\-h elp] [\-\-] cpxfile
+.IP
+cpxfiddle options:
+.TP
+\fB\-w\fR width
+of complexfile in complex pixels
+.TP
+\fB\-f\fR format
+of complex input file.
+ci2|cr4|cr8 (cr4 is default)
+r4 now also possible, though it limites other options.
+do not use subsampling, mirroring etc, file is cat\-ed.
+.TP
+\fB\-q\fR output
+what is to be computed
+mag|phase|real|imag|normal (mag is default)
+.TP
+\fB\-e\fR exp
+compute scale*output^exp
+.TP
+\fB\-s\fR scale
+compute scale*output^exp
+.TP
+\fB\-l\fR firstline
+cut out complexfile from firstline
+.TP
+\fB\-L\fR lastline
+cut out complexfile up to lastline
+.HP
+\fB\-p\fR firstpixel cut out complexfile from firstpixel
+.TP
+\fB\-P\fR lastpixel
+cut out complexfile up to lastpixel
+.TP
+\fB\-m\fR X Y XY
+mirror option.
+.TP
+\fB\-M\fR 1/1
+multilook factor in X/Y direction
+.TP
+\fB\-F\fR 1/1
+subsample Factor in X/Y direction
+.IP
+GMT options:
+.TP
+\fB\-T\fR title
+title to plot (one word only for now)
+default no title
+.TP
+\fB\-c\fR colortable name of color table (see grd2cpt)
+if \fB\-q\fR mag then gray table is default
+if \fB\-q\fR other then gray table is default
+.TP
+\fB\-S\fR
+add a scale bar (psscale)
+.TP
+\fB\-Z\fR
+continuous color table (grd2cpt)
+.TP
+\fB\-K\fR
+Leave postscript file open after last call to GMT
+.TP
+\fB\-z\fR cm
+largest size of paper
+.TP
+\fB\-U\fR
+Place UNIX time stamp and filename in output
+.IP
+General options:
+.TP
+\fB\-g\fR
+Do not call gv to view result.
+.TP
+\fB\-o\fR
+output postscript file, default=23819.eps (pid)
+.TP
+\fB\-G\fR
+output grd file, default=23819.eps (pid)
+If specified, file is not removed at end
+If file exists, prompted for reuse.
+.TP
+\fB\-C\fR
+output cpt file, default=23819.cpt (pid)
+If specified, file is not removed at end
+If file exists, prompted for reuse.
+.TP
+\fB\-V\fR erbose
+give verbose information
+.TP
+\fB\-h\fR elp
+this help
+.TP
+complexfile
+inputfile, major row order pixel interleaved
+.IP
+EXAMPLES:
+.IP
+Generate a postscript file with phase of complex interferogram
+in file cpxint.raw (complex 2x4B floats) that has 998 range pixels:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qphase\fR \fB\-fcr4\fR \fB\-\-\fR cpxint.raw
+.IP
+The same but with a scale bar, timestamp, and no title:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qphase\fR \fB\-fcr4\fR \fB\-Tnone\fR \fB\-U\fR \fB\-S\fR \fB\-\-\fR cpxint.raw
+.IP
+To plot the magnitude to the power 0.3 of a file in the format
+complex short integers (2x2B) use:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qmag\fR \fB\-fci2\fR \fB\-e0\fR.3 \fB\-\-\fR cpxint.raw
+.IP
+To see a large file it is convenient to set a large size (\fB\-z\fR).
+This file cannot be printed, but viewing it with gv is nice:
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-qphase\fR \fB\-z200\fR \fB\-\-\fR cpxint.raw
+.IP
+To plot the phase of a hgt file, first create a tmp file with
+the program hgt2file (hgtfile infile linelength tmpfile [ampflag])
+Next, run cpx2ps with appropriate flags for a float file, e.g.
+(Note that this limits some options in scaling etc.):
+.IP
+cpx2ps \fB\-w\fR 998 \fB\-crainbow\fR \fB\-fr4\fR \fB\-\-\fR tmpfile
+.IP
+BUGS:
+.IP
+When mirroring and multilooking/subsampling sometimes
+the number of lines/pixels of the output is computed
+incorrectly. Simply don't use multilooking/subsampling...
+.IP
+Please mail bugs/comments to kampes at geo.tudelft.nl
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, GMT
+.SH "SEE ALSO"
+The full documentation for
+.B cpx2ps
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B cpx2ps
+programs are properly installed at your site, the command
+.IP
+.B info cpx2ps
+.PP
+should give you access to the complete manual.
diff --git a/debian/doris.1 b/debian/man/doris.1
similarity index 100%
rename from debian/doris.1
rename to debian/man/doris.1
diff --git a/debian/man/doris.adddummystep.sh.1 b/debian/man/doris.adddummystep.sh.1
new file mode 100644
index 0000000..5a3db2d
--- /dev/null
+++ b/debian/man/doris.adddummystep.sh.1
@@ -0,0 +1,106 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH DORIS.ADDDUMMYSTEP.SH "1" "September 2017" "doris.adddummystep.sh " "User Commands"
+.SH NAME
+doris.adddummystep.sh \- manual page for doris.adddummystep.sh
+.SH DESCRIPTION
+USAGE: doris.adddummystep.sh <doris_process_name> <.res>
+.TP
+EX: doris.adddummystep.sh coarse_correl
+master_slave.res
+.TP
+doris.adddummystep.sh
+resample slave.res
+.SS "Doris process names by order:"
+.TP
+1.
+precise_orbits 14. resample
+.TP
+2.
+crop 15. interfero
+.TP
+3.
+sim_amplitude 16. comp_refphase
+.TP
+4.
+master_timing 17. subtr_refphase
+.TP
+5.
+filt_azi 18. comp_refdem
+.TP
+6.
+filt_range 19. subtr_refdem
+.TP
+7
+oversample 20. coherence
+.TP
+8.
+coarse_orbits 21. filtphase
+.TP
+9.
+coarse_correl 22. unwrap
+.PP
+10. fine_coreg 23. slant2h
+11. timing_error 24. geocoding
+12. dem_assist 25. dinsar
+13. comp_coregpm 26. <extra>
+.IP
+Thank you for using Doris!
+.IP
+TU Delft \- DEOS Radar Group 2011
+.PP
+USAGE: doris.adddummystep.sh <doris_process_name> <.res>
+.TP
+EX: doris.adddummystep.sh coarse_correl
+master_slave.res
+.TP
+doris.adddummystep.sh
+resample slave.res
+.SS "Doris process names by order:"
+.TP
+1.
+precise_orbits 14. resample
+.TP
+2.
+crop 15. interfero
+.TP
+3.
+sim_amplitude 16. comp_refphase
+.TP
+4.
+master_timing 17. subtr_refphase
+.TP
+5.
+filt_azi 18. comp_refdem
+.TP
+6.
+filt_range 19. subtr_refdem
+.TP
+7
+oversample 20. coherence
+.TP
+8.
+coarse_orbits 21. filtphase
+.TP
+9.
+coarse_correl 22. unwrap
+.PP
+10. fine_coreg 23. slant2h
+11. timing_error 24. geocoding
+12. dem_assist 25. dinsar
+13. comp_coregpm 26. <extra>
+.IP
+Thank you for using Doris!
+.IP
+TU Delft \- DEOS Radar Group 2011
+.SH "SEE ALSO"
+The full documentation for
+.B doris.adddummystep.sh
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B doris.adddummystep.sh
+programs are properly installed at your site, the command
+.IP
+.B info doris.adddummystep.sh
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/doris.rmstep.sh.1 b/debian/man/doris.rmstep.sh.1
new file mode 100644
index 0000000..7ceebfb
--- /dev/null
+++ b/debian/man/doris.rmstep.sh.1
@@ -0,0 +1,106 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH DORIS.RMSTEP.SH "1" "September 2017" "doris.rmstep.sh " "User Commands"
+.SH NAME
+doris.rmstep.sh \- manual page for doris.rmstep.sh
+.SH DESCRIPTION
+USAGE: doris.rmstep.sh <doris_process_name> <.res>
+.TP
+EX: doris.rmstep.sh coarse_correl
+master_slave.res
+.TP
+doris.rmstep.sh
+resample slave.res
+.SS "Doris process names by order:"
+.TP
+1.
+precise_orbits 14. resample
+.TP
+2.
+crop 15. interfero
+.TP
+3.
+sim_amplitude 16. comp_refphase
+.TP
+4.
+master_timing 17. subtr_refphase
+.TP
+5.
+filt_azi 18. comp_refdem
+.TP
+6.
+filt_range 19. subtr_refdem
+.TP
+7
+oversample 20. coherence
+.TP
+8.
+coarse_orbits 21. filtphase
+.TP
+9.
+coarse_correl 22. unwrap
+.PP
+10. fine_coreg 23. slant2h
+11. timing_error 24. geocoding
+12. dem_assist 25. dinsar
+13. comp_coregpm 26. <extra>
+.IP
+Thank you for using Doris!
+.IP
+TU Delft \- DEOS Radar Group 2011
+.PP
+USAGE: doris.rmstep.sh <doris_process_name> <.res>
+.TP
+EX: doris.rmstep.sh coarse_correl
+master_slave.res
+.TP
+doris.rmstep.sh
+resample slave.res
+.SS "Doris process names by order:"
+.TP
+1.
+precise_orbits 14. resample
+.TP
+2.
+crop 15. interfero
+.TP
+3.
+sim_amplitude 16. comp_refphase
+.TP
+4.
+master_timing 17. subtr_refphase
+.TP
+5.
+filt_azi 18. comp_refdem
+.TP
+6.
+filt_range 19. subtr_refdem
+.TP
+7
+oversample 20. coherence
+.TP
+8.
+coarse_orbits 21. filtphase
+.TP
+9.
+coarse_correl 22. unwrap
+.PP
+10. fine_coreg 23. slant2h
+11. timing_error 24. geocoding
+12. dem_assist 25. dinsar
+13. comp_coregpm 26. <extra>
+.IP
+Thank you for using Doris!
+.IP
+TU Delft \- DEOS Radar Group 2011
+.SH "SEE ALSO"
+The full documentation for
+.B doris.rmstep.sh
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B doris.rmstep.sh
+programs are properly installed at your site, the command
+.IP
+.B info doris.rmstep.sh
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/doris.slant2h4master.sh.1 b/debian/man/doris.slant2h4master.sh.1
new file mode 100644
index 0000000..7d0c7a6
--- /dev/null
+++ b/debian/man/doris.slant2h4master.sh.1
@@ -0,0 +1,21 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH USAGE: "1" "September 2017" "Usage: doris.slant2h4master.sh <interferometric.res> <radarcodedDEM.raw>" "User Commands"
+.SH NAME
+Usage: \- manual page for Usage: doris.slant2h4master.sh <interferometric.res> <radarcodedDEM.raw>
+.SH SYNOPSIS
+.B doris.slant2h4master.sh
+\fI\,<interferometric.res> <radarcodedDEM.raw>\/\fR
+.SH DESCRIPTION
+
+.SH "SEE ALSO"
+The full documentation for
+.B Usage:
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B Usage:
+programs are properly installed at your site, the command
+.IP
+.B info Usage:
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/gammaReadfiles.csh.1 b/debian/man/gammaReadfiles.csh.1
new file mode 100644
index 0000000..1f144fd
--- /dev/null
+++ b/debian/man/gammaReadfiles.csh.1
@@ -0,0 +1,37 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH GAMMAREADFILES.CSH "1" "September 2017" "gammaReadfiles.csh" "User Commands"
+.SH NAME
+gammaReadfiles.csh \- import form Gamma format
+.SH DESCRIPTION
+.IP
+USAGE:gammaReadfiles.csh processParameterFile sensorParameterFile slcFile
+.IP
+where
+processParameterFile is the gamma SLC processing par file (pXXX.slc.par, or XXX.pslcpar)
+sensorParameterFile is the gamma sensor par file (ERS1_ESA.par, or System.par)
+slcfile is the complex SAR image file in 2 bytes integer format (CI2).
+.IP
+EXAMPLE:
+.IP
+gammaReadfiles.csh p20070105.slc.par System.par 20070105.slc
+.IP
+where
+processParameterFile is the gamma SLC processing par file (pXXX.slc.par, or XXX.pslcpar)
+sensorParameterFile is the gamma sensor par file (ERS1_ESA.par, or System.par)
+slcfile is the complex SAR image file in 2 bytes integer format (CI2).
+.IP
+EXAMPLE:
+.IP
+gammaReadfiles.csh p20070105.slc.par System.par 20070105.slc
+.SH "SEE ALSO"
+The full documentation for
+.B gammaReadfiles.csh
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B gammaReadfiles.csh
+programs are properly installed at your site, the command
+.IP
+.B info gammaReadfiles.csh
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/getorb_rs2.py.1 b/debian/man/getorb_rs2.py.1
new file mode 100644
index 0000000..252f062
--- /dev/null
+++ b/debian/man/getorb_rs2.py.1
@@ -0,0 +1,25 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH GETTING "1" "September 2017" "Getting precise orbits for Radarsat2" "User Commands"
+.SH NAME
+Getting \- manual page for Getting precise orbits for Radarsat2
+.SH DESCRIPTION
+Getting precise orbits for Radarsat2
+orbit dir: None
+resfile: None
+extratime: 16
+.PP
+orbit dir: None
+resfile: None
+extratime: 16
+.SH "SEE ALSO"
+The full documentation for
+.B Getting
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B Getting
+programs are properly installed at your site, the command
+.IP
+.B info Getting
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/heightamb.1 b/debian/man/heightamb.1
new file mode 100644
index 0000000..c745de7
--- /dev/null
+++ b/debian/man/heightamb.1
@@ -0,0 +1,83 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH HEIGHTAMB "1" "September 2017" "heightamb v1.1, BK software, Bert Kampes, (c)1999-2000" "User Commands"
+.SH NAME
+heightamb \- icompute height ambiguity for flat terrain
+.SH DESCRIPTION
+heightamb v1.1, BK software, Bert Kampes, (c)1999\-2000
+.IP
+Computes indicative height ambiguity for flat terrain
+as function of perpendicular baseline. A larger Bperp
+yields more sensitivity to height, i.e., a decreasing
+height ambiguity (the height difference corresponding
+to a 2pi phase difference (a fringe)).
+.PP
+Program parameters (ERS):
+.TP
+lambda:
+0.0565646 [m]
+.TP
+R1:
+850000.0 [m]
+.TP
+theta:
+23.0 [deg]
+.TP
+theta:
+[rad]
+.TP
+terrain slope:
+0.0 [rad]
+.SS "EXAMPLES:"
+.IP
+heightamb
+heightamb 100
+heightamb 25 50 100 200 400 800
+.PP
+Input perp. Baseline [m]:
+.PP
+Bperp = [m] \fB\-\-\-\fR> Height ambiguity = [m/2pi]
+.IP
+Computes indicative height ambiguity for flat terrain
+as function of perpendicular baseline. A larger Bperp
+yields more sensitivity to height, i.e., a decreasing
+height ambiguity (the height difference corresponding
+to a 2pi phase difference (a fringe)).
+.PP
+Program parameters (ERS):
+\fB\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\-\fR
+.TP
+lambda:
+0.0565646 [m]
+.TP
+R1:
+850000.0 [m]
+.TP
+theta:
+23.0 [deg]
+.TP
+theta:
+[rad]
+.TP
+terrain slope:
+0.0 [rad]
+.SS "EXAMPLES:"
+.IP
+heightamb
+heightamb 100
+heightamb 25 50 100 200 400 800
+.PP
+Input perp. Baseline [m]:
+.PP
+Bperp = [m] \fB\-\-\-\fR> Height ambiguity = [m/2pi]
+.SH "SEE ALSO"
+The full documentation for
+.B heightamb
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B heightamb
+programs are properly installed at your site, the command
+.IP
+.B info heightamb
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/lonlatCoh2ascii.1 b/debian/man/lonlatCoh2ascii.1
new file mode 100644
index 0000000..4606c09
--- /dev/null
+++ b/debian/man/lonlatCoh2ascii.1
@@ -0,0 +1,120 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH LONLATCOH2ASCII "1" "September 2017" "lonlatCoh2ascii v1.0 Doris software, TUDelft, (c)1999-2011" "User Commands"
+.SH NAME
+lonlatCoh2ascii \- create 3 column ASCII files from the binary doris output
+.SH DESCRIPTION
+lonlatCoh2ascii v1.0 Doris software, TUDelft, (c)1999\-2011
+.IP
+SYNOPSIS:
+.TP
+lonlatCoh2ascii
+longitude_file latitude_file Coh_file output_Coh_file
+.IP
+This csh\-script creates a 3 column ASCII file with "lon lat coh"
+from the binary doris output (matrices) after step geocode.
+It filters out invalid data, indicated with "\-999" by Doris.
+.IP
+The output file can be used further with GMT to create a grd file.
+The format of the 3 input files are matrices in real4 float format.
+all of the same size. They describe the irregular geocoded position
+of the pixels in the interferogram, and the corresponding heights.
+.IP
+The steps taken are within this script:
+.IP
+1) Create 3 temporary ASCII files with all data in a single
+.IP
+large column using cpxfiddle program;
+.IP
+2) Create two 3 column ASCII file (lon lat ***)
+.IP
+using "paste";
+.IP
+3) remove \fB\-999\fR invalid data using "grep"
+4) Tidy up, remove temp files.
+.TP
+These steps may take a while.
+Obviously staying in binary format
+.TP
+would be better.
+This script is intented to work on all platforms,
+.IP
+and to be straightforward and understandable, rather than ingenious.
+.IP
+DEPENDENCIES:
+.IP
+cpxfiddle program, part of Doris distribution.
+grep utility, standard UNIX
+paste utility, standard UNIX
+Note that lambda=longitude; phi=latitude
+.IP
+EXAMPLE:
+.TP
+lonlatCoh2ascii Outdata/lambda.raw Outdata/phi.raw Outdata/Coherence.raw
+lonlatcoh.dat
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, paste, grep, http://gmt.soest.hawaii.edu/
+.IP
+SYNOPSIS:
+.TP
+lonlatCoh2ascii
+longitude_file latitude_file Coh_file output_Coh_file
+.IP
+This csh\-script creates a 3 column ASCII file with "lon lat coh"
+from the binary doris output (matrices) after step geocode.
+It filters out invalid data, indicated with "\-999" by Doris.
+.IP
+The output file can be used further with GMT to create a grd file.
+The format of the 3 input files are matrices in real4 float format.
+all of the same size. They describe the irregular geocoded position
+of the pixels in the interferogram, and the corresponding heights.
+.IP
+The steps taken are within this script:
+.IP
+1) Create 3 temporary ASCII files with all data in a single
+.IP
+large column using cpxfiddle program;
+.IP
+2) Create two 3 column ASCII file (lon lat ***)
+.IP
+using "paste";
+.IP
+3) remove \fB\-999\fR invalid data using "grep"
+4) Tidy up, remove temp files.
+.TP
+These steps may take a while.
+Obviously staying in binary format
+.TP
+would be better.
+This script is intented to work on all platforms,
+.IP
+and to be straightforward and understandable, rather than ingenious.
+.IP
+DEPENDENCIES:
+.IP
+cpxfiddle program, part of Doris distribution.
+grep utility, standard UNIX
+paste utility, standard UNIX
+Note that lambda=longitude; phi=latitude
+.IP
+EXAMPLE:
+.TP
+lonlatCoh2ascii Outdata/lambda.raw Outdata/phi.raw Outdata/Coherence.raw
+lonlatcoh.dat
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, paste, grep, http://gmt.soest.hawaii.edu/
+.SH "SEE ALSO"
+The full documentation for
+.B lonlatCoh2ascii
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B lonlatCoh2ascii
+programs are properly installed at your site, the command
+.IP
+.B info lonlatCoh2ascii
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/lonlathei2ascii.1 b/debian/man/lonlathei2ascii.1
new file mode 100644
index 0000000..41e3dc8
--- /dev/null
+++ b/debian/man/lonlathei2ascii.1
@@ -0,0 +1,120 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH LONLATHEI2ASCII "1" "September 2017" "lonlathei2ascii v1.0 Doris software, bert kampes, (c)1999-2003" "User Commands"
+.SH NAME
+lonlathei2ascii \- create 3 column ASCII files from the binary doris output
+.SH DESCRIPTION
+lonlathei2ascii v1.0 Doris software, bert kampes, (c)1999\-2003
+.IP
+SYNOPSIS:
+.TP
+lonlathei2ascii
+longitude_file latitude_file height_file output_file
+.IP
+This csh\-script creates an 3 column ASCII file with "lon lat hei"
+from the binary doris output (matrices) after step geocode.
+It filters out invalid data, indicated with "\-999" by Doris.
+.IP
+The output file can be used further with GMT to create a grd file.
+The format of the 3 input files are matrices in real4 float format.
+all of the same size. They describe the irregular geocoded position
+of the pixels in the interferogram, and the corresponding heights.
+.IP
+The steps taken are within this script:
+.IP
+1) Create 3 temporary ASCII files with all data in a single
+.IP
+large column using cpxfiddle program;
+.IP
+2) Create a single 3 column ASCII file (lon lat hei)
+.IP
+using "paste";
+.IP
+3) remove \fB\-999\fR invalid data using "grep"
+4) Tidy up, remove temp files.
+.TP
+These steps may take a while.
+Obviously staying in binary format
+.TP
+would be better.
+This script is intented to work on all platforms,
+.IP
+and to be straightforward and understandable, rather than ingenious.
+.IP
+DEPENDENCIES:
+.IP
+cpxfiddle program, part of Doris distribution.
+grep utility, standard UNIX
+paste utility, standard UNIX
+Note that lambda=longitude; phi=latitude
+.IP
+EXAMPLE:
+.TP
+lonlathei2ascii Outdata/lambda.raw Outdata/phi.raw Outdata/heights.raw
+lonlathei.dat
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, paste, grep, http://gmt.soest.hawaii.edu/
+.IP
+SYNOPSIS:
+.TP
+lonlathei2ascii
+longitude_file latitude_file height_file output_file
+.IP
+This csh\-script creates an 3 column ASCII file with "lon lat hei"
+from the binary doris output (matrices) after step geocode.
+It filters out invalid data, indicated with "\-999" by Doris.
+.IP
+The output file can be used further with GMT to create a grd file.
+The format of the 3 input files are matrices in real4 float format.
+all of the same size. They describe the irregular geocoded position
+of the pixels in the interferogram, and the corresponding heights.
+.IP
+The steps taken are within this script:
+.IP
+1) Create 3 temporary ASCII files with all data in a single
+.IP
+large column using cpxfiddle program;
+.IP
+2) Create a single 3 column ASCII file (lon lat hei)
+.IP
+using "paste";
+.IP
+3) remove \fB\-999\fR invalid data using "grep"
+4) Tidy up, remove temp files.
+.TP
+These steps may take a while.
+Obviously staying in binary format
+.TP
+would be better.
+This script is intented to work on all platforms,
+.IP
+and to be straightforward and understandable, rather than ingenious.
+.IP
+DEPENDENCIES:
+.IP
+cpxfiddle program, part of Doris distribution.
+grep utility, standard UNIX
+paste utility, standard UNIX
+Note that lambda=longitude; phi=latitude
+.IP
+EXAMPLE:
+.TP
+lonlathei2ascii Outdata/lambda.raw Outdata/phi.raw Outdata/heights.raw
+lonlathei.dat
+.IP
+SEE ALSO:
+.IP
+cpxfiddle, paste, grep, http://gmt.soest.hawaii.edu/
+.SH "SEE ALSO"
+The full documentation for
+.B lonlathei2ascii
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B lonlathei2ascii
+programs are properly installed at your site, the command
+.IP
+.B info lonlathei2ascii
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/phasefilt.doris.1 b/debian/man/phasefilt.doris.1
new file mode 100644
index 0000000..d2e9c6a
--- /dev/null
+++ b/debian/man/phasefilt.doris.1
@@ -0,0 +1,135 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH PHASEFILT.DORIS "1" "September 2017" "phasefilt.doris v1.1, FMR software, Bert Kampes, (c)2000\n" "User Commands"
+.SH NAME
+phasefilt.doris \- Filter mph file using Doris
+.SH DESCRIPTION
+phasefilt.doris v1.1, FMR software, Bert Kampes, (c)2000
+.TP
+SYNOPSIS:
+.IP
+phasefilt.doris \fB\-l\fR numlines [\-o .filtered] [\-a 0.25] [\-e 3]
+.IP
+[\-b 32] [\-m goldstein] [\-k kernel | \fB\-K\fR file] [\-\-] infile
+.IP
+OPTIONS:
+.TP
+\fB\-l\fR numlines
+Number of lines in inputfile.
+.TP
+\fB\-m\fR method
+method either: "goldstein", "spectral", or "spatialconv".
+.TP
+\fB\-o\fR filename
+Output file name.
+.TP
+\fB\-a\fR A
+Alpha filter parameter A e{0,1} (Goldstein method).
+.TP
+\fB\-e\fR E
+Use overlap of 2*E pixels, so partially the same
+complex data are used to estimate the spectrum.
+.TP
+\fB\-b\fR B
+Filter in blocks of size (B,B). Should be power of 2.
+.TP
+\fB\-k\fR kernel
+1D KERNEL, use underscores for space. For example
+\fB\-k\fR 5_1_2_3_4_5
+.TP
+\fB\-K\fR file
+Name of ascii input file containing a 2D kernel for
+method spatialconv or spectral. 1 header line with:
+"height", "width" and "scalefactor", for example:
+.TP
+3 3 0.111111111111
+1 1 1
+1 1 1
+1 1 1
+.TP
+infile
+Name of input file with numlines (complexr4).
+.IP
+BUGS:
+.IP
+\-
+.IP
+EXAMPLES:
+.IP
+\-
+.IP
+SEE ALSO:
+.IP
+Doris user's manual, e.g. online, at: www.geo.tudelft.nl/doris/
+.PP
+infile: does not exist
+.TP
+PROGRAM:
+phasefilt.doris \fB\-\-\fR Filter mph file using Doris.
+.IP
+SYNOPSIS:
+.IP
+phasefilt.doris \fB\-l\fR numlines [\-o .filtered] [\-a 0.25] [\-e 3]
+.IP
+[\-b 32] [\-m goldstein] [\-k kernel | \fB\-K\fR file] [\-\-] infile
+.IP
+OPTIONS:
+.TP
+\fB\-l\fR numlines
+Number of lines in inputfile.
+.TP
+\fB\-m\fR method
+method either: "goldstein", "spectral", or "spatialconv".
+.TP
+\fB\-o\fR filename
+Output file name.
+.TP
+\fB\-a\fR A
+Alpha filter parameter A e{0,1} (Goldstein method).
+.TP
+\fB\-e\fR E
+Use overlap of 2*E pixels, so partially the same
+complex data are used to estimate the spectrum.
+.TP
+\fB\-b\fR B
+Filter in blocks of size (B,B). Should be power of 2.
+.TP
+\fB\-k\fR kernel
+1D KERNEL, use underscores for space. For example
+\fB\-k\fR 5_1_2_3_4_5
+.TP
+\fB\-K\fR file
+Name of ascii input file containing a 2D kernel for
+method spatialconv or spectral. 1 header line with:
+"height", "width" and "scalefactor", for example:
+.TP
+3 3 0.111111111111
+1 1 1
+1 1 1
+1 1 1
+.TP
+infile
+Name of input file with numlines (complexr4).
+.IP
+BUGS:
+.IP
+\-
+.IP
+EXAMPLES:
+.IP
+\-
+.IP
+SEE ALSO:
+.IP
+Doris user's manual, e.g. online, at: www.geo.tudelft.nl/doris/
+.SH "SEE ALSO"
+The full documentation for
+.B phasefilt.doris
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B phasefilt.doris
+programs are properly installed at your site, the command
+.IP
+.B info phasefilt.doris
+.PP
+should give you access to the complete manual.
diff --git a/debian/plotcpm.1 b/debian/man/plotcpm.1
similarity index 100%
rename from debian/plotcpm.1
rename to debian/man/plotcpm.1
diff --git a/debian/man/plotcpm.erroffsets.1 b/debian/man/plotcpm.erroffsets.1
new file mode 100644
index 0000000..b776ee9
--- /dev/null
+++ b/debian/man/plotcpm.erroffsets.1
@@ -0,0 +1,92 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH PLOTCPM.ERROFFSETS "1" "September 2017" "plotcpm.erroffsets v1.3, FMR software, TUDelft Radar Group (c)1999-2008" "User Commands"
+.SH NAME
+plotcpm.erroffsets \- plot error offset data from Doris
+.SH DESCRIPTION
+plotcpm.erroffsets v1.3, FMR software, TUDelft Radar Group (c)1999\-2008
+.IP
+input file: CPM_Data cannot be read.
+.IP
+plotcpm.erroffsets \fB\-\-\fR program to plot data from Doris
+.IP
+Usage:
+.IP
+plotcpm.erroffsets [[[ifile [linelo hi pixlo hi [slcfile]]]
+.IP
+tip: plotcpm.erroffsets CPM_Data 1 25000 1 4900 slcfile.raw
+.TP
+infile
+is a data file from doris, see this script for details.
+.TP
+linelo
+is first line.
+.TP
+linehi
+is last line.
+.IP
+pixello is first pixel.
+pixello is last pixel.
+slcfile is filename of SLC data for background of magnitude.
+.IP
+format must be ci2 or cr4 of SLC data.
+.IP
+Defaults:
+.TP
+ifile
+== CPM_Data
+.IP
+linelo == 1
+linehi == 25000
+pixlo == 1
+pixhi == 4900
+.IP
+If magnitude background calls to GMT and cpxfiddle.
+.IP
+input file: CPM_Data cannot be read.
+.IP
+plotcpm.erroffsets \fB\-\-\fR program to plot data from Doris
+.IP
+Usage:
+.IP
+plotcpm.erroffsets [[[ifile [linelo hi pixlo hi [slcfile]]]
+.IP
+tip: plotcpm.erroffsets CPM_Data 1 25000 1 4900 slcfile.raw
+.TP
+infile
+is a data file from doris, see this script for details.
+.TP
+linelo
+is first line.
+.TP
+linehi
+is last line.
+.IP
+pixello is first pixel.
+pixello is last pixel.
+slcfile is filename of SLC data for background of magnitude.
+.IP
+format must be ci2 or cr4 of SLC data.
+.IP
+Defaults:
+.TP
+ifile
+== CPM_Data
+.IP
+linelo == 1
+linehi == 25000
+pixlo == 1
+pixhi == 4900
+.IP
+If magnitude background calls to GMT and cpxfiddle.
+.SH "SEE ALSO"
+The full documentation for
+.B plotcpm.erroffsets
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B plotcpm.erroffsets
+programs are properly installed at your site, the command
+.IP
+.B info plotcpm.erroffsets
+.PP
+should give you access to the complete manual.
diff --git a/debian/plotoffsets.1 b/debian/man/plotoffsets.1
similarity index 100%
rename from debian/plotoffsets.1
rename to debian/man/plotoffsets.1
diff --git a/debian/man/rs2_dump_data.py.1 b/debian/man/rs2_dump_data.py.1
new file mode 100644
index 0000000..2e0855e
--- /dev/null
+++ b/debian/man/rs2_dump_data.py.1
@@ -0,0 +1,78 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH RS2_DUMP_DATA.PY "1" "September 2017" "rs2_dump_data.py " "User Commands"
+.SH NAME
+rs2_dump_data.py \- manual page for rs2_dump_data.py
+.SH DESCRIPTION
+Error : Unrecognized input or missing arguments
+.PP
+INFO : @(#)Doris InSAR software, $Revision: 1.1 $, $Author: TUDelft $
+.PP
+Usage : rs2_dump_data.py <inputfile> <outputfile> [l0 lN p0 pN] [\-res RESFILE]
+.TP
+inputfile
+is the input Radarsat\-2 geotiff filename : master.tif
+.TP
+outputfile
+is the output filename : master.slc
+.TP
+l0
+is the first azimuth line (starting at 1)
+.TP
+lN
+is the last azimuth line
+.TP
+p0
+is the first range pixel (starting at 1)
+.TP
+pN
+is the last range pixel
+.TP
+RESFILE
+DORIS result file that is to be updated for crop metadata (optional)
+.IP
+This software is part of Doris InSAR software package.
+.PP
+(c) 1999\-2010 Delft University of Technology, the Netherlands.
+.PP
+Error : Unrecognized input or missing arguments
+.PP
+INFO : @(#)Doris InSAR software, $Revision: 1.1 $, $Author: TUDelft $
+.PP
+Usage : rs2_dump_data.py <inputfile> <outputfile> [l0 lN p0 pN] [\-res RESFILE]
+.TP
+inputfile
+is the input Radarsat\-2 geotiff filename : master.tif
+.TP
+outputfile
+is the output filename : master.slc
+.TP
+l0
+is the first azimuth line (starting at 1)
+.TP
+lN
+is the last azimuth line
+.TP
+p0
+is the first range pixel (starting at 1)
+.TP
+pN
+is the last range pixel
+.TP
+RESFILE
+DORIS result file that is to be updated for crop metadata (optional)
+.IP
+This software is part of Doris InSAR software package.
+.PP
+(c) 1999\-2010 Delft University of Technology, the Netherlands.
+.SH "SEE ALSO"
+The full documentation for
+.B rs2_dump_data.py
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B rs2_dump_data.py
+programs are properly installed at your site, the command
+.IP
+.B info rs2_dump_data.py
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/rs2_dump_header2doris.py.1 b/debian/man/rs2_dump_header2doris.py.1
new file mode 100644
index 0000000..4d80ec8
--- /dev/null
+++ b/debian/man/rs2_dump_header2doris.py.1
@@ -0,0 +1,40 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH RS2_DUMP_HEADER2DORIS.PY "1" "September 2017" "rs2_dump_header2doris.py " "User Commands"
+.SH NAME
+rs2_dump_header2doris.py \- manual page for rs2_dump_header2doris.py
+.SH DESCRIPTION
+Error : Unrecognized input or missing arguments
+.PP
+INFO : @(#)Doris InSAR software, $Revision: 1.2 $, $Author: TUDelft $
+.PP
+Usage : python rs2_dump_header2doris.py rs2_XML_product > outputfile
+.IP
+where rs2_XML_product is the input filename
+.IP
+This software is part of Doris InSAR software package.
+.PP
+(c) 1999\-2010 Delft University of Technology, the Netherlands.
+.PP
+Error : Unrecognized input or missing arguments
+.PP
+INFO : @(#)Doris InSAR software, $Revision: 1.2 $, $Author: TUDelft $
+.PP
+Usage : python rs2_dump_header2doris.py rs2_XML_product > outputfile
+.IP
+where rs2_XML_product is the input filename
+.IP
+This software is part of Doris InSAR software package.
+.PP
+(c) 1999\-2010 Delft University of Technology, the Netherlands.
+.SH "SEE ALSO"
+The full documentation for
+.B rs2_dump_header2doris.py
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B rs2_dump_header2doris.py
+programs are properly installed at your site, the command
+.IP
+.B info rs2_dump_header2doris.py
+.PP
+should give you access to the complete manual.
diff --git a/debian/rundoris.1 b/debian/man/rundoris.1
similarity index 100%
rename from debian/rundoris.1
rename to debian/man/rundoris.1
diff --git a/debian/man/tsx_dump_data.py.1 b/debian/man/tsx_dump_data.py.1
new file mode 100644
index 0000000..0f267b6
--- /dev/null
+++ b/debian/man/tsx_dump_data.py.1
@@ -0,0 +1,63 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH UNRECOGNIZED "1" "September 2017" "Unrecognized input" "User Commands"
+.SH NAME
+Unrecognized \- manual page for Unrecognized input
+.SH SYNOPSIS
+.B python
+\fI\,tsx_dump_data.py tsx_COSAR_product outputfile \/\fR[\fI\,l0 lN p0 pN\/\fR] \fI\,-res RESFILE\/\fR
+.SH DESCRIPTION
+Unrecognized input
+.IP
+where tsx_COSAR_product is the input filename
+.TP
+outputfile
+is the output filename
+.TP
+l0
+is the first azimuth line (starting at 1)
+.TP
+lN
+is the last azimuth line
+.TP
+p0
+is the first range pixel (starting at 1)
+.TP
+pN
+is the last range pixel
+.TP
+RESFILE
+DORIS result file that is to be updated for crop metadata
+.PP
+Usage: python tsx_dump_data.py tsx_COSAR_product outputfile [l0 lN p0 pN] \fB\-res\fR RESFILE
+.IP
+where tsx_COSAR_product is the input filename
+.TP
+outputfile
+is the output filename
+.TP
+l0
+is the first azimuth line (starting at 1)
+.TP
+lN
+is the last azimuth line
+.TP
+p0
+is the first range pixel (starting at 1)
+.TP
+pN
+is the last range pixel
+.TP
+RESFILE
+DORIS result file that is to be updated for crop metadata
+.SH "SEE ALSO"
+The full documentation for
+.B Unrecognized
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B Unrecognized
+programs are properly installed at your site, the command
+.IP
+.B info Unrecognized
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/tsx_dump_header2doris.py.1 b/debian/man/tsx_dump_header2doris.py.1
new file mode 100644
index 0000000..3400ee5
--- /dev/null
+++ b/debian/man/tsx_dump_header2doris.py.1
@@ -0,0 +1,27 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH UNRECOGNIZED "1" "September 2017" "Unrecognized input" "User Commands"
+.SH NAME
+Unrecognized \- manual page for Unrecognized input
+.SH SYNOPSIS
+.B python
+\fI\,tsx_dump_header2doris.py tsx_XML_product > outputfile\/\fR
+.SH DESCRIPTION
+Unrecognized input
+.IP
+where tsx_XML_product is the input filename
+.PP
+Usage: python tsx_dump_header2doris.py tsx_XML_product > outputfile
+.IP
+where tsx_XML_product is the input filename
+.SH "SEE ALSO"
+The full documentation for
+.B Unrecognized
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B Unrecognized
+programs are properly installed at your site, the command
+.IP
+.B info Unrecognized
+.PP
+should give you access to the complete manual.
diff --git a/debian/man/viewanddel.1 b/debian/man/viewanddel.1
new file mode 100644
index 0000000..5f91745
--- /dev/null
+++ b/debian/man/viewanddel.1
@@ -0,0 +1,23 @@
+.\" DO NOT MODIFY THIS FILE! It was generated by help2man 1.47.4.
+.TH VIEWANDDEL "1" "September 2017" "viewanddel file.ps" "User Commands"
+.SH NAME
+viewanddel \- view a temporary PS file and then delete it
+.SH DESCRIPTION
+bin/viewanddel file.ps
+View a temporary postscript file and
+then delete it afterwards.
+.PP
+View a temporary postscript file and
+then delete it afterwards.
+.SH "SEE ALSO"
+The full documentation for
+.B viewanddel
+is maintained as a Texinfo manual. If the
+.B info
+and
+.B viewanddel
+programs are properly installed at your site, the command
+.IP
+.B info viewanddel
+.PP
+should give you access to the complete manual.
diff --git a/debian/manpages b/debian/manpages
index bae3056..2802b76 100644
--- a/debian/manpages
+++ b/debian/manpages
@@ -1,4 +1,26 @@
-debian/doris.1
-debian/rundoris.1
-debian/plotcpm.1
-debian/plotoffsets.1
+debian/man/doris.1
+debian/man/rundoris.1
+debian/man/plotcpm.1
+debian/man/plotoffsets.1
+debian/man/ascii2ascii_UTM.1
+debian/man/ascii2grdAutoMinMaxHDR.1
+debian/man/ascii2ps.1
+debian/man/baseline.doris.sh.1
+debian/man/coregpm.doris.1
+debian/man/cpx2ps.1
+debian/man/doris.adddummystep.sh.1
+debian/man/doris.rmstep.sh.1
+debian/man/doris.slant2h4master.sh.1
+debian/man/gammaReadfiles.csh.1
+debian/man/getorb_rs2.py.1
+debian/man/heightamb.1
+debian/man/lonlatCoh2ascii.1
+debian/man/lonlathei2ascii.1
+debian/man/phasefilt.doris.1
+debian/man/plotcpm.erroffsets.1
+debian/man/rs2_dump_data.py.1
+debian/man/rs2_dump_header2doris.py.1
+debian/man/tsx_dump_data.py.1
+debian/man/tsx_dump_header2doris.py.1
+debian/man/viewanddel.1
+
--
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