-
RCRYST
-
rcryst n
Will compute the discrepancy (computed as a R factor) between the
current experimental nOe build-up curves, and the build-up curve as
analysed from the last LP analysis.
see also : CALIBDI
DIST
RELAXRATE
-
READ
-
READ file_name
Reads the file as the new data set in standard format .
Same as READC
see also : build2d
build3d
READH
READL
READM
READS
READT
READV
READZ
WRITE
-
READC
-
Same as READ
-
READH
-
READH file_name
Will read ft-nmr compatible files.
see also : READ
WRITEH
-
READL
-
Load NMR1/NMR2 data-set
see also : READ
WRITEL
-
READM
-
READM file_name
Loads a file created with the program MATLAB, using the -ascii
option; or with the WRITEM command.
see also : READ
WRITEM
-
READS
-
READS filename
Read from the disk in standard compact format. This format is
compatible among incompatible platforms. It is ASCII format and can
even be E_Mailed.
see also : READ
READT
WRITES
-
READT
-
READT filename
Read from the disk in text format. The data are in formatted values,
1 entry per line. Useful for entering data from an other program.
see also : READ
READS
WRITET
-
READV
-
Load Varian data set.
see also : READ
-
READZ
-
READZ filename
Reads from the disk in compacted file format.
see also : ORDER
READ
WRITEZ
-
REAL
-
REAL {Fx}
This command extract the real part of the current the data set
considered as complex.
On 2D and 3D you can choose on which axis the REAL operation will be
taken. Data size can thus be reduced either by 2 , 4 or even 8.
see also : FLIP
FLOP
ITYPE
MODULUS
-
REF
-
This command will force a new computing of the display, as if a
display command had been issued. This is useful for cleaning the
spectrum after any command that draw on the spectrum, such as POINT,
SHOWLINE, etc...
see also : CDISP2D
DISP1D
DISP2D
REF3D
REFMACRO
UNREF
-
REF3D
-
This command will display a 3D view of the current 3D data-set, in
the window previously opened with the DISP3D command. The parameters
used for the display can be chosen with the DISP3D? and the CHECK3D
commands.
see also : CHECK3D
DISP3D
-
REFMACRO
-
When this context is set to 1 the program refreshes the on-
screen display during macro execution, this permits to follow the
data during the program execution, but slows down the macro
execution.
When equal to 0, the display is refreshed only at the end of the
macro execution. Default value is 0.
see also : CLEAR
REF
UNREF
-
RELAXRATE
-
Compute the relaxation rate (in arbitrary unit) from the last LP
analysis.
see also : CALIBDI
DIST
METH
ORDER
RCRYST
RT->PK
SLOPE
-
rem_h2o
-
rem_h2o -no param-
this macro will remove most of water signal (large zero-frequency
signal) by fitting and removing the water FID in the time domain
used in 1D, will overflow the 2D area !!
to be used before any processing, on the FID.
-
RESIDUE
-
Returns into the current buffer the result of the substraction of
the DATA buffer, with the reconstruction of the mock data from the
spectrum held into the current buffer. To be used after a MaxEnt run
to see that part of the signal not analysed by the MaxEnt process.
see also : GET
MAXENT
SHOW
-
REVERSE
-
REVERSE {Fx}
reverse the order of the current data-set (i.e. first points are
last, last points are first).
If dataset is complex, REVERSE will reverse the complex vector (2
by 2).
see also : INVF
REVF
TRANSPOSE
-
REVF
-
REVF {Fx}
Processes FID data-sets by multiplying by -1 2 points out of 4.
Permits to preprocess Bruker FIDs in Dim 2 (Bruker trick) before
RFT, or permits to bring back zero frequency in the center for some
other data formats
see also : FT
INVF
ITYPE
REVERSE
-
RFT
-
RFT {Fx}
Perform real-to-complex Fourier Transform on data
see also : FT
-
rm
-
as in unix
see also : CD
ls
more
pwd
SH
vi
vim
vip
-
ROTATE
-
ROTATE 0 / 1
When ROTATE=1, plots are rotated by 90 degrees, useful for plotting
1D spectra on A4 Postscript plotter or on a A3 HP-GL plotter
see also : PLOT
-
ROW
-
ROW n
Extract the nth 1D row (along F2) from the 2D data-set, and put it
in the 1D buffer. The row will be available as a 1D data set when
going from 2D to 1D
see also : COL
colint
DIM
PLANE
rowint
VERT
-
rowint
-
interactive
permits to choose rows interactively on a 2D by clicking on the data-set
see also : COL
colint
ph2dc
planeint
ROW
vertint
-
rshift
-
rshift n_points
makes a right shift of the data
see also : CHSIZE
EXTRACT
lshift
-
RT->AR
-
RT->AR n
Compute back the autoregressive coefficients from a given set of
roots.
n = 1 : forward coefficients are calculated from forward roots
n = 2 : backward coefficients are calculated from backward roots
n = 3 : both coefficient sets are calculated
see also : AR->RT
ORDER
RT->PK
RTCLEAN
RTINV
RTLIST
RTMATCH
RTPIV
RTREFLECT
RTSELECT
-
RT->PK
-
RT->PK size n delay
Calculate the peaks parameters from the roots by a least-square
method, computed on the size first points of the current data-set.
This is the fourth (and last) step of the LP-SVD method.
n = 1 : forward roots
n = 2 : "matched" roots
delay is the dead-time delay of the first point .in seconds. (the
error on the time zero)
see also : AR->RT
ORDER
RT->AR
RTCLEAN
RTINV
RTLIST
RTMATCH
RTPIV
RTREFLECT
RTSELECT
-
RTCLEAN
-
RTCLEAN n
Keep only the roots whose modulus is greater than one. Useful to
clean up root-set computed from a backward analysis, before
inverting.
n = 1 : forward roots
n = 2 : backward roots
see also : AR->RT
ORDER
RT->AR
RT->PK
RTINV
RTLIST
RTMATCH
RTPIV
RTREFLECT
RTSELECT
-
RTINV
-
RTINV n
Calculate the inverse conjugate of all the polynomial roots, thus
converting backward and forward polynomial. To be used after a
backward analysis.
n = 1 : forward roots are inversed, and their inverses are put in
the backward root array.
n = 2 : backward roots are inversed, and their inverses are put in
the forward root array.
see also : AR->RT
ORDER
RT->AR
RT->PK
RTCLEAN
RTLIST
RTMATCH
RTPIV
RTREFLECT
RTSELECT
-
RTLIST
-
RTLIST n i j
List the roots of prediction-error polynomial from entry i to entry
j.
n = 1 : forward roots
n = 2 : backward roots
n = 3 : matched roots
see also : AR->RT
RT->AR
RT->PK
RTCLEAN
RTINV
RTMATCH
RTPIV
RTREFLECT
RTSELECT
-
RTMATCH
-
RTMATCH nsignals
"Match" the forward and backward roots to eliminate the roots dues
to noise. Those matched roots can then be used by RT->PK, with the
"matched forward & backward" roots. nsignals is the number of true
roots expected.
see also : AR->RT
ORDER
RT->AR
RT->PK
RTCLEAN
RTINV
RTLIST
RTPIV
RTREFLECT
RTSELECT
-
RTPIV
-
RTPIV alpha
Will remove all the forward roots with frequency higher than 1/alpha
(in -PI +PI unit). Used to remove spurious frequency when doing
build-up curve analysis.
see also : AR->RT
RT->AR
RT->PK
RTCLEAN
RTINV
RTLIST
RTMATCH
RTREFLECT
RTSELECT
-
RTREFLECT
-
RTREFLECT n
Calculate the inverse conjugate of roots lying outside the unity
circle. The modified roots are let in the same root array.
n = 1 : forward roots
n = 2 : backward roots
see also : AR->RT
ORDER
RT->AR
RT->PK
RTCLEAN
RTINV
RTLIST
RTMATCH
RTPIV
RTSELECT
-
RTSELECT
-
RTSELECT n index()
Select the roots whose index() are given. To end selection, enter
the index 0.
n = 1 : forward roots
n = 2 : backward roots
n = 3 : matched roots
see also : AR->RT
ORDER
RT->AR
RT->PK
RTCLEAN
RTINV
RTLIST
RTMATCH
RTPIV
RTREFLECT
-
RZOOM
-
This command permits, when in zoom mode in 2D, to jump to a zoom
window symmetric relatively to the diagonal of the one currently
used.
see also : ZM
ZOOM