Provided by: spd_1.3.0-1ubuntu3_amd64 
NAME
spd - SPatial Distortion Program
SYNOPSIS
Synchrotron image corrections and azimuthal integration
DESCRIPTION
SPD stands for SPatial Distortion. Written in C language, this command-line driven program
deals with images coming from X-ray diffusion/diffraction experiments. It does
subsequently:
* intensity corrections (dark current, flat field correction, ...),
* geometry corrections using spline files or a pair of distortion arrays,
* azimuthal integration in 2D or 1D after masking defective pixels. SPD was originally
written by Jorg Klora for ESRF and was re-written by Peter Boesecke from ESRF/ID02.
Maintenance and packaging of the program are provided by Rainer Wilcke and Jerome Kieffer
from SciSoft at ESRF.
OPTIONS
Usage: spd [--server] [--exit] parameter=option [filenames]
src_id=<source image shared memory id>
src_ext=<source image file extension> (default none)
cor_id=<shared memory id of corrected image>
cor_ext=<corrected image file extension> (default none)
type=<output data type> (default "FloatIEEE32")
dvo=<value> data value offset (default 0)
dark_id=<dark image shared memory id>
dark_file=<dark image file name>
dark_const=<value> subtract constant dark image value default: no dark image
subtraction done
dark_ext=<dark image file extension> default none
do_dark=0|1 if 0, suppress dark image correction default 1
save_dark=0|1|2 save dark image memory to file
0: never, 1: always, 2: only if new (default 2)
inp_const=<value> add input image constant (default 0.)
inp_exp=<value> apply exponent to input image (default 1.)
inp_factor=<value> multiply with input image factor (default 1.)
raw_cmpr="none"|"gzip"|"z" compression of raw & dark images (default none)
flood_id=<flood field image shared memory id> (or flat field)
flood_file=<flood field image file name> (default: no flood field used)
bckg_id=<scattering background image shared memory id>
bckg_file=<scattering background image file name> (default: no scattering background used)
bckg_const=<additive scattering constant> (default 0.)
bckg_fact=<constant scattering factor> (default 1.)
header_id=<shared memory id for data header> (default: not used)
pass=0|1 pass input file header to output (default 0)
header_min=<minimum header length for output file> (default 0)
header_ext=<extension for header output file> (default none)
distortion_file=<file> (default "spatial.dat")
xfile=<file> (x distortion read from edf file)
yfile=<file> (y distortion read from edf file)
xoutfile=<file> (x distortion saved to edf file)
youtfile=<file> (y distortion saved to edf file)
active_radius=<value> (values outside will not be corrected)
precen_1=xxx for pre-rotation center_1 (default calculated)
precen_2=xxx for pre-rotation center_2 (default calculated)
predis=xxx for pre-rotation distance (default calculated)
prerot_1=<angle (rad) for pre-rotation around axis 1> (default 0.)
prerot_2=<angle (rad) for pre-rotation around axis 2> (default 0.)
prerot_3=<angle (rad) for pre-rotation around axis 3> (default 0.)
psize_distort=0|1|2 take image params from distortion file 0: none, 1: pix, 2: pix, cen,
dis, proj, rot (default 0)
cen_1=xxx if set, defines Center_1 header value
cen_2=xxx if set, defines Center_2 header value
i0=xxx if set, defines Intensity0 header value
i1=xxx if set, defines Intensity1 header value
off_1=xxx if set, defines Offset_1 header value
off_2=xxx if set, defines Offset_2 header value
pix_1=xxx if set, defines PSize_1 header value
pix_2=xxx if set, defines PSize_2 header value
bis_1=xxx if set, defines BSize_1 header value
bis_2=xxx if set, defines BSize_2 header value
dis=xxx if set, defines SampleDistance header value
ori=xxx if set, defines RasterOrientation header value
tit=xxx if set, defines Title header value
wvl=xxx if set, defines WaveLength header value
pro="Saxs"|"Waxs" projection type of image (default Saxs)
rot_1=<angle (rad) for detector rotation plane 1> (default 0.)
rot_2=<angle (rad) for detector rotation plane 2> (default 0.)
rot_3=<angle (rad) for detector rotation plane 3> (default 0.)
base_name=<name> (default "image")
outdir=<pathname> directory for output files (default: base_name)
verbose=-1|0|1|2 message printing level (low -> high, default 1)
version=0|1 print version string of the program if != 0
simul=0|1 (default 0)
do_distortion=0|1|2|3 distortion correction (default 1) (0: none, 1: after dark, 2:
after flat, 3: after norm)
flat_distortion=0|1 normalize to flat imgage (default 1)
do_prerotation=0|1|2 pre-rotation correction (default 1) (0: none, 1: after, 2:
without distortion correction)
norm_int=0|1 intensity normalization (default 0 = no)
norm_factor=<intensity normalization factor> (default 1.)
overflow=xxx (default 0 = not set)
dummy=<value> (default 0. = not set)
inp_min=<value> (default 0. = not set)
inp_max=<value> (default 0. = not set)
bin_1=<value> factor for x-binning (default 1 = no binning)
bin_2=<value> factor for y-binning (default 1 = no binning)
azim_int=0|1 azimuthal regrouping (default 0 = no)
azim_pass=0|1 pass full header to azimuthal regrouping (def. 1 = yes)
azim_pro="Saxs"|"Waxs" project. type of azim. regrp. (default Saxs)
azim_id=<shared memory id of regrouped image> (default -1)
azim_ext=<file extension of regrouped image> (default none)
azim_r0=<value> minimum regrouping radius (default 0.)
azim_r_num=<value> radial output size (default 0)
azim_a0=<degrees> 1st regrouping start angle (default 0.)
azim_a1=<degrees> 2nd regrouping start angle (default: not used)
azim_da=<degrees> angular regrouping interval (default 1.)
azim_a_num=<value> angular output size (default 0)
ave_id=<shared memory id of averaged image> (default -1)
ave_ext=<file extension of averaged image> (default none)
ave_scf=<scale factor for "s" values> (default 1.)
mask_file=<azimuthal regrouping mask file name>
(default: not used)
--server switch to server mode, i.e. wait for
new command/image to process on stdin
--exit quit the program when we are on server mode.
BUGS
Azimuthal integration can only be achieved if a wavelength is given, even if it is not
needed for any calculation.
SPD was developed at ESRF and is tightly bound to Spec shared-memory arrays
(http://www.certif.com) and EDF (ESRF Data Format) images, both in input and output.