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Sandra Loss, Rainer Kerssebaum, Bruker BioSpin
Tips and Tricks(for Acquisition & Processing - leading to good spectra)
Innovation with Integrity La Jolla, September 2016
2Bruker Users Meeting @SMASH, La Jolla, September 2016
Topics
• Window Functions
• Spectral Resolution and Zero Filling
• Folding and Filters
• Forward Linear Prediction
• Backward Linear Prediction
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Window Functions
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Basics
time domain frequency domain
FT
decay lineshape
amplitude integral
period frequency
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Lineshape
FT
FT
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Window Function
• The intensity of each FID-datapoint is multiplied with a intensity
value defined by the window function
• Application:
sensitivity gain
enhancement of resolution
dealing with truncation artifacts
interesting signals may be increased, non-interesting
suppressed (example: COSY-diagonal)
without window function exponential function gaussian function
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Sensitivity Gain - Exponential Function
• Improvement of signal to noise with an exponential function:
beginning of FID: dominated by signal
end of FID: dominated by noise
WDW: EM LB > 0 (speed of decay of exponential)
processing with EFP
no
window
function
exponential
function
FT
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• Improvement of resolution with Gaussian function:
slow decay of FID: sharp line(s)
fast decay of FID: broad line(s)
WDW: GM LB < 0 0 < GB < 1 (defines position of maximum)
processing with GFP
Improvement of Resolution - Gaussian Func.
8
Gaussian
function
FT
no
window
function
9Bruker Users Meeting @SMASH, La Jolla, September 2016
• Improvement of Resolution without S/N loss with Traficante function:
WDW: TRAF 0 < LB < 1
Traficante
function
FT
Improvement of Resolution – Traficante Func.
no
windows
function
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Spectral Resolution and Zero Filling
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Spectral Resolution
AQ
DW AQ = DW*TD
AQ = TD/(2*SWH)
DW = 1/(2*SWH)
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Spectral Resolution
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Important Parameters
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Spectral Resolution
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Spectral Resolution
TD
t
TDeff
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Zero-filling
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TD = 64k
SI = 32 k
TD = 64k
SI = 64k
TD = 64k
SI = 128k
Zero-filling
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Spectral Resolution
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Folding and Filtering
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Folding
Nyquist theorem: min. 2 datapoints / period must be sampled
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Folding
sw
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Antialiasing Filter
sw
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Oversampling and digital Filter
AQ = DW*TD DW = 1/(2*SWH)
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Oversampling and digital Filter
AQ = DW*TD AQ = TD/(2*SWH)
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Oversampling and digital Filter
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Oversampling and digital Filter
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Quantitation Noise
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Quantitation Noise
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Quantitation Noise
rg = 1
rg = 57
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Forward Linear Prediction
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Forward Linear Prediction
• only for truncated FID
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Forward Linear Prediction
t
si
tdeff lpbin
• only for truncated FID
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Example: Forward Linear Prediction: HSQC
ppm
5.56.06.57.07.58.08.59.09.510.010.5 ppm
105
110
115
120
125
130
Current Data Parameters
NAME TXI_Calb_0102
EXPNO 10
PROCNO 1
F2 - Acquisition Parameters
Date_ 20020110
Time 4.03INSTRUM spectPROBHD 5mm TXI 1H-13C
PULPROG invif3gpsi
TD 2048
SOLVENT H2ONS 2
DS 8
SWH 8012.820 HzFIDRES 3.912510 Hz
AQ 0.1279076 secRG 512
DW 62.400 usec
DE 4.50 usec
TE 296.4 KCEN_HN1 0.00001523 sec
CEN_HN2 0.00003045 secCNST4 94.0000000
d0 0.00000300 sec
D1 1.00000000 sec
d11 0.03000000 sec
d13 0.00000400 sec
D16 0.00010000 secD24 0.00265957 sec
d26 0.00265957 secDELTA 0.00112250 sec
DELTA1 0.00110800 sec
IN0 0.00025000 sec
l3 128
======== CHANNEL f1 ========
NUC1 1H
P1 8.25 usecp2 16.50 usec
P28 1000.00 usec
PL1 0.00 dB
SFO1 500.1323506 MHz
======== CHANNEL f3 ========
CPDPRG3 garp64
NUC3 15N
P21 38.70 usecp22 77.40 usec
PCPD3 250.00 usec
PL3 -3.00 dBPL16 12.90 dBSFO3 50.6837130 MHz
====== GRADIENT CHANNEL =====
GPNAM1 SINE.100GPNAM2 SINE.100
GPNAM3 SINE.100GPX1 0.00 %
GPX2 0.00 %
GPX3 0.00 %
GPY1 0.00 %
GPY2 0.00 %
GPY3 0.00 %GPZ1 50.00 %
GPZ2 80.00 %GPZ3 8.10 %
P16 1000.00 usec
F1 - Acquisition parametersND0 2
TD 239
SFO1 50.68371 MHz
FIDRES 8.368201 Hz
SW 39.460 ppmFnMODE Echo-Antiecho
F2 - Processing parameters
SI 512SF 500.1300000 MHz
WDW SINE
SSB 2
LB 0.00 HzGB 0
PC 4.00
F1 - Processing parameters
SI 1024
MC2 echo-antiecho
SF 50.6777330 MHz
WDW SINE
SSB 2
LB 0.00 Hz
GB 0
1H-15N HSQC Calbindin D9k
ns=2
34Bruker Users Meeting @SMASH, La Jolla, September 2016
678910 ppm
256
678910 ppm
128
678910 ppm
64
horizontal projection (1H) No measured increments
No measured increments has no influence onto the resolution in the direct
dimension - S/N increases with TD[F1]
Example: Forward Linear Prediction: HSQC
35Bruker Users Meeting @SMASH, La Jolla, September 2016
vertical projection (15N) No measured increments
256
105110115120125130 ppm
128
105110115120125130 ppm105110115120125130 ppm
64
vertical projection: experimental data without linear prediction
Example: Forward Linear Prediction: HSQC
36Bruker Users Meeting @SMASH, La Jolla, September 2016
105110115120125130 ppm
LPFC
LPBIN=192
64 + 192
64 + 192
vertical projection (15N) No measured increments
105110115120125130 ppm105110115120125130 ppm
LPFC
LPBIN=0
64 + 64
105110115120125130 ppm
64
256
Example: Forward Linear Prediction: HSQC
37Bruker Users Meeting @SMASH, La Jolla, September 2016
678910 ppmLPFC
LPBIN=0
64 + 192
678910 ppmLPFC
LPBIN=0
64 + 64
Example: Forward Linear Prediction: HSQC
256
678910 ppm678910 ppm
64
TD[F1] 256 vs. 64 + LPfc
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Forward Linear Prediction: Parameters
• ME_mod: LPfc (method: real time data)
LPmifc (constant time data)
• TDeff: number of used FID-points
TDeff = 0 TDeff = TD
• LPBIN: number of points after prediction
LPBIN = 0 LPBIN = TD (or TDeff)
• NCOEF: number of coefficients for prediction function
LPBIN points need at least 3 for each signal: frequency,
amplitude, relaxation
• SI: number of real datapoints after processing
t
si
tdeff lpbin
39Bruker Users Meeting @SMASH, La Jolla, September 2016
Forward Linear Prediction: Parameters
• LPBIN: 0 (double number of points)
Maximum: X * TD (or X * TDeff)
• NCOEF: 3 … 256 (number of signals * 3)
indirect dimension:
maximum number of signals
in one column * 3
typical values and limits
t
si
tdeff lpbin
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Backward Linear Prediction
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Backward Linear Prediction
• is used if datapoints at the beginning of the FID are distorted
(this typically leads to baseline distortions)
42Bruker Users Meeting @SMASH, La Jolla, September 2016
Backward Linear Prediction
• is used if datapoints at the beginning of the FID are distorted
(this typically leads to baseline distortions)
43Bruker Users Meeting @SMASH, La Jolla, September 2016
Backward Linear Prediction
• first datapoints need to be corrected
lpbin
t
td
tdoff
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Backward Linear Prediction
• digitally filtered data need to be converted into “analog” type data using
command “convdta”
convdta
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Backward Linear Prediction: Parameters
• ME_mod: LPbc (method)
• TDeff: number of used datapoints
TDeff = 0 TDeff = TD
• TDOFF: number of points to be replaced
(negative value: additional points)
should be even (complex data)
• LPBIN: number of input points for calculation
• NCOEF: number of coefficients in function for calculation of LPBIN
datapoints (für each signal 3: frequency, amplitude,
relaxation)
46Bruker Users Meeting @SMASH, La Jolla, September 2016
Backward Linear Prediction: Parameters
• TDOFF: 8 … 128
• LPBIN: 1k … 8k
• NCOEF: 30 … 2k (number of signals * 3)
typical values and limits
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Backward Linear Prediction: Parameters
48Bruker Users Meeting @SMASH, La Jolla, September 2016
Backward Linear Prediction: Parameters
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Innovation with Integrity
Copyright © 2016 Bruker Corporation. All rights reserved. www.bruker.com
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