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commit b51757d4065fd2b68eeabf317f1da5882fa18c60 Author: Antonio Valentino <[email protected]> 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 <[email protected]> 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 <[email protected]> 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 [email protected] +.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 [email protected] +.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 + -- Alioth's /usr/local/bin/git-commit-notice on /srv/git.debian.org/git/pkg-grass/doris.git _______________________________________________ Pkg-grass-devel mailing list [email protected] http://lists.alioth.debian.org/cgi-bin/mailman/listinfo/pkg-grass-devel
